GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Abstract

We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1${\mathrm{M}}_{\odot }$ during the first and second observing runs of the Advanced gravitational-wave detector network. During the first observing run (O1), from September $12^{\mathrm{th}}$, 2015 to January $19^{\mathrm{th}}$, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run (O2), which ran from November $30^{\mathrm{th}}$, 2016 to August $25^{\mathrm{th}}$, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary black hole mergers, four of which we report here for the first time: GW170729, GW170809, GW170818 and GW170823. For all significant gravitational-wave events, we provide estimates of the source properties. The detected binary black holes have total masses between $18.6_{-0.7}^{+3.2}{\mathrm{M}}_{\odot }$, and $84.4_{-11.1}^{+15.8}{\mathrm{M}}_{\odot }$, and range in distance between $320_{-110}^{+120}$ Mpc and $2840_{-1360}^{+1400}$ Mpc. No neutron star - black hole mergers were detected. In addition to highly significant gravitational-wave events, we also provide a list of marginal event candidates with an estimated false alarm rate less than 1 per 30 days. From these results over the first two observing runs, which include approximately one gravitational-wave detection per 15 days of data searched, we infer merger rates at the 90% confidence intervals of $110-3840$ ${\mathrm{Gpc}}^{-3}{\mathrm{y}}^{-1}$ for binary neutron stars and $9.7-101$ ${\mathrm{Gpc}}^{-3}{\mathrm{y}}^{-1}$ for binary black holes assuming fixed population distributions, and determine a neutron star - black hole merger rate 90% upper limit of $610$ ${\mathrm{Gpc}}^{-3}{\mathrm{y}}^{-1}$.

arXiv commentTotal: 49 pages and 17 figures. Strain data are available from the Gravitational Wave Open Science Center at https://doi.org/10.7935/82H3-HH23. Figures, data behind the figures, including posterior samples, are available from https://dcc.ligo.org/LIGO-P1800307/public

References in corpus (213)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• A Massive Pulsar in a Compact Relativistic Binary
• Multi-messenger Observations of a Binary Neutron Star Merger
• Advanced LIGO
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• GW170817: Measurements of Neutron Star Radii and Equation of State
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Tests of general relativity with GW150914
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Evolution of Binary Black Hole Spacetimes
• Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
• Effective one-body approach to general relativistic two-body dynamics
• Gravitational wave extraction from an inspiraling configuration of merging black holes
• Properties of the binary neutron star merger GW170817
• GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Interferometer design of the KAGRA gravitational wave detector
• Properties of the Binary Black Hole Merger GW150914
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system
• Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
• Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Transition from inspiral to plunge in binary black hole coalescences
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
• Coalescing binary systems of compact objects to (post)$^{5/2}-Newtonian order. V. Spin Effects
• GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
• Compact Object Modeling with the StarTrack Population Synthesis Code
• An Effective Field Theory of Gravity for Extended Objects
• Observing binary inspiral in gravitational radiation: One interferometer
• Pulsational Pair-Instability Supernovae
• A simple model of complete precessing black-hole-binary gravitational waveforms
• The Black Hole Mass Distribution in the Galaxy
• The PyCBC search for gravitational waves from compact binary coalescence
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
• On The Maximum Mass of Stellar Black Holes
• A new route towards merging massive black holes
• Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian order
• The Mass Distribution of Stellar-Mass Black Holes
• Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
• GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
• Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
• Total recoil: the maximum kick from nonspinning black-hole binary inspiral
• The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
• Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• A catalog of 174 binary black-hole simulations for gravitational-wave astronomy
• Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Rapid Bayesian position reconstruction for gravitational-wave transients
• The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• A chi-squared time-frequency discriminator for gravitational wave detection
• Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order
• Measuring the neutron star equation of state with gravitational wave observations
• Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE
• Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
• Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
• Approximate Universal Relations for Neutron Stars and Quark Stars
• Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
• Spinning-black-hole binaries: The orbital hang up
• The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
• Systematic parameter errors in inspiraling neutron star binaries
• Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms
• Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO
• On the Mass Distribution and Birth Masses of Neutron Stars
• Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
• Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
• Networks of gravitational wave detectors and three figures of merit
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• Dimensional regularization of the gravitational interaction of point masses
• Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• Coherent method for detection of gravitational wave bursts
• Distinguishing Spin-Aligned and Isotropic Black Hole Populations With Gravitational Waves
• Effective One Body description of tidal effects in inspiralling compact binaries
• Are LIGO's Black Holes Made From Smaller Black Holes?
• BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
• Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
• Gravitational waves from inspiraling compact binaries: The quadrupole-moment term
• Mass Measurements of Black Holes in X-Ray Transients: Is There a Mass Gap?
• Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization
• Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations
• Modeling the dynamics of tidally-interacting binary neutron stars up to merger
• An improved analytical description of inspiralling and coalescing black-hole binaries
• The final spin from binary black holes in quasi-circular orbits
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Spin-Orbit Misalignment in Close Binaries with Two Compact Objects
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects
• Estimating the final spin of a binary black hole coalescence
• Detecting binary compact-object mergers with gravitational waves: Understanding and Improving the sensitivity of the PyCBC search
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
• 1-OGC: The first open gravitational-wave catalog of binary mergers from analysis of public Advanced LIGO data
• Compact Binary Coalescences in the Band of Ground-based Gravitational-Wave Detectors
• Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
• Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
• Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
• Observing gravitational-wave transient GW150914 with minimal assumptions
• Where are LIGO's Big Black Holes?
• Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
• LISA observations of rapidly spinning massive black hole binary systems
• Determining the population properties of spinning black holes
• The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
• Triangulation of gravitational wave sources with a network of detectors
• Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• Degeneracy between mass and spin in black-hole-binary waveforms
• Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
• Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
• Addressing the spin question in gravitational-wave searches: Waveform templates for inspiralling compact binaries with nonprecessing spins
• The environment of the binary neutron star merger GW170817
• Source localization with an advanced gravitational wave detector network
• Use of gravitational waves to probe the formation channels of compact binaries
• Dimensional regularization of the third post-Newtonian gravitational wave generation from two point masses
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Next-to-next-to-leading order spin-orbit effects in the gravitational wave flux and orbital phasing of compact binaries
• The last orbit of binary black holes
• Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
• Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
• Black Hole and Neutron Star Binary Mergers in Triple Systems: Merger Fraction and Spin-Orbit Misalignment
• Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
• Measuring the spin of black holes in binary systems using gravitational waves
• Using spin to understand the formation of LIGO's black holes
• Self-interaction spin effects in inspiralling compact binaries
• The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• Effects of waveform model systematics on the interpretation of GW150914
• Multi-timescale analysis of phase transitions in precessing black-hole binaries
• Effects of Data Quality Vetoes on a Search for Compact Binary Coalescences in Advanced LIGO's First Observing Run
• Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
• A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
• Distance measures in gravitational-wave astrophysics and cosmology
• Gravitational-Wave Astronomy with Inspiral Signals of Spinning Compact-Object Binaries
• Quasiuniversal properties of neutron star mergers
• Accuracy of inference on the physics of binary evolution from gravitational-wave observations
• Observing and measuring the neutron-star equation-of-state in spinning binary neutron star systems
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's first observing run
• Counting And Confusion: Bayesian Rate Estimation With Multiple Populations
• Parameter estimation of spinning binary inspirals using Markov-chain Monte Carlo
• Improving the Sensitivity of Advanced LIGO Using Noise Subtraction
• Implications of PSR J0737-3039B for the Galactic NS-NS Binary Merger Rate
• Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
• Low-Latency Gravitational Wave Alerts for Multi-Messenger Astronomy During the Second Advanced LIGO and Virgo Observing Run
• Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO
• Gravitational-wave luminosity of binary neutron stars mergers
• Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
• Fast evaluation of multi-detector consistency for real-time gravitational wave searches
• Distinguishing compact binary population synthesis models using gravitational-wave observations of coalescing binary black holes
• What if LIGO's gravitational wave detections are strongly lensed by massive galaxy clusters?
• Remnant of binary black-hole mergers: New simulations and peak luminosity studies
• Basic Parameter Estimation of Binary Neutron Star Systems by the Advanced LIGO/Virgo Network
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Can we measure individual black-hole spins from gravitational-wave observations?
• Distinguishing short duration noise transients in LIGO data to improve the PyCBC search for gravitational waves from high mass binary black hole mergers
• Dynamics of stellar black holes in young star clusters with different metallicities - I. Implications for X-ray binaries
• Estimating parameters of coalescing compact binaries with a detector network including LIGO Australia
• Parameter estimation for heavy binary-black holes with networks of second-generation gravitational-wave detectors
• Estimating parameters of coalescing compact binaries with proposed advanced detector networks
• Audio-band frequency-dependent squeezing
• Reconstructing the calibrated strain signal in the Advanced LIGO detectors
• Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes
• Precessional dynamics of black hole triples: binary mergers with near-zero effective spin
• Impact of Bayesian prior on the characterization of binary black hole coalescences
• Construction of KAGRA: an Underground Gravitational Wave Observatory
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Spin-Orbit Misalignment of Merging Black-Hole Binaries with Tertiary Companions
• On the accuracy and precision of numerical waveforms: Effect of waveform extraction methodology
• Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• Effects of nonquadrupole modes in the detection and parameter estimation of black hole binaries with nonprecessing spins
• Parameter estimation on gravitational waves from neutron-star binaries with spinning components
• Comparison of Gravitational Wave Detector Network Sky Localization Approximations
• Localization of short duration gravitational-wave transients with the early advanced LIGO and Virgo detectors
• On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors
• Spin-Precession: Breaking the Black Hole--Neutron Star Degeneracy
• Characterising Transient Noise in the LIGO Detectors
• A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model
• Bayesian inference on compact binary inspiral gravitational radiation signals in interferometric data
• Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
• Constraining black-hole spins with gravitational wave observations
• Future prospects for ground-based gravitational wave detectors $-$ The Galactic double neutron star merger rate revisited
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• The coalescence remnant of spinning binary black holes
• Measuring intermediate mass black hole binaries with advanced gravitational wave detectors
• Testing the validity of the single-spin approximation in inspiral-merger-ringdown waveforms
• Designing a template bank to observe compact binary coalescences in Advanced LIGO's second observing run
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity
• Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances
• A more effective coordinate system for parameter estimation of precessing compact binaries from gravitational waves
• Estimating parameters of binary black holes from gravitational-wave observations of their inspiral, merger and ringdown
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• Impact of precession on aligned-spin searches for neutron-star--black-hole binaries
• Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression
• Data Quality Studies of Enhanced Interferometric Gravitational Wave Detectors
• Characterization of low-significance gravitational-wave compact binary sources

Cited by in corpus (2486)

• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Science Case for the Einstein Telescope
• Constraints on Primordial Black Holes
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
• Observation of gravitational waves from two neutron star-black hole coalescences
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• IceCube-Gen2: The Window to the Extreme Universe
• Teleparallel Gravity: From Theory to Cosmology
• Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
• Kilonovae
• The SXS Collaboration catalog of binary black hole simulations
• Surrogate models for precessing binary black hole simulations with unequal masses
• Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Formation and Evolution of Compact Object Binaries in AGN Disks
• Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory
• A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
• AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
• New binary black hole mergers in the second observing run of Advanced LIGO and Advanced Virgo
• Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
• The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background
• AION: An Atom Interferometer Observatory and Network
• Concepts and status of Chinese space gravitational wave detection projects
• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• Formation and Evolution of Primordial Black Hole Binaries in the Early Universe
• IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
• New Horizons for Fundamental Physics with LISA
• One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
• GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal
• COSMIC Variance in Binary Population Synthesis
• The effect of the metallicity-specific star formation history on double compact object mergers
• Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
• Surrogate model of hybridized numerical relativity binary black hole waveforms
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Neutron star tidal deformability and equation of state constraints
• Conservative Dynamics of Binary Systems to Third Post-Minkowskian Order from the Effective Field Theory Approach
• Merging black holes in young star clusters
• Black hole ringdown: the importance of overtones
• Multi-messenger Bayesian parameter inference of a binary neutron-star merger
• Real-time gravitational-wave science with neural posterior estimation
• Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
• 2-OGC: Open Gravitational-wave Catalog of binary mergers from analysis of public Advanced LIGO and Virgo data
• Constraints on the cosmic expansion history from GWTC-3
• Did NANOGrav see a signal from primordial black hole formation?
• Rates of Compact Object Coalescences
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Stationary black holes and light rings
• 4-OGC: Catalog of gravitational waves from compact-binary mergers
• LIGO Detector Characterization in the Second and Third Observing Runs
• Black hole superradiance of self-interacting scalar fields
• GW190521 as a merger of Proca stars: a potential new vector boson of $8.7\times 10^{-13}$ eV
• Cosmic Conundra Explained by Thermal History and Primordial Black Holes
• Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
• The Threshold for Primordial Black Hole Formation: a Simple Analytic Prescription
• Gravitational waves from a universe filled with primordial black holes
• Constraints from gravitational wave detections of binary black hole mergers on the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ rate
• Modeling Dense Star Clusters in the Milky Way and Beyond with the $\text{CMC}$ Cluster Catalog
• FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
• Lower bound on the primordial black hole merger rate
• Bayesian parameter estimation using conditional variational autoencoders for gravitational-wave astronomy
• An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451
• Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory
• Two populations of LIGO-Virgo black holes
• Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5M_{\odot }$ Compact Object and a Neutron Star
• Novel black-bounce spacetimes: wormholes, regularity, energy conditions, and causal structure
• Observational Evidence for Primordial Black Holes: A Positivist Perspective
• A wide star-black-hole binary system from radial-velocity measurements
• 3-OGC: Catalog of gravitational waves from compact-binary mergers
• Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform
• GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• BlackHawk v2.0: A public code for calculating the Hawking evaporation spectra of any black hole distribution
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• Primordial Black Holes as Dark Matter Candidates
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio
• Pulsar Timing Array Constraints on Primordial Black Holes with NANOGrav 11-Year Data Set
• Gravitational waves from extreme-mass-ratio systems in astrophysical environments
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• Spontaneous scalarisation of charged black holes: coupling dependence and dynamical features
• New binary black hole mergers in the LIGO--Virgo O3a data
• A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• Fundamental physics implications on higher-curvature theories from the binary black hole signals in the LIGO-Virgo Catalog GWTC-1
• Multi-Messenger Astrophysics
• Gravitational-wave parameter estimation with autoregressive neural network flows
• The impact of pair-instability mass loss on the binary black hole mass distribution
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Strong gravitational lensing of explosive transients
• The BayesWave analysis pipeline in the era of gravitational wave observations
• Fast Radio Bursts from Magnetars Born in Binary Neutron Star Mergers and Accretion Induced Collapse
• Beyond the Standard Models with Cosmic Strings
• Primordial black hole formation by vacuum bubbles
• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties
• Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and ${}^{12}$C($\alpha$, $\gamma$)${}^{16}$O rate on the pair-instability black hole mass gap
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Analysis of Ringdown Overtones in GW150914
• Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
• Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
• Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
• The redshift evolution of the binary black hole merger rate: a weighty matter
• Novel approach to binary dynamics: application to the fifth post-Newtonian level
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian
• On the Rate of Neutron Star Binary Mergers from Globular Clusters
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run
• Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
• Second-order self-force calculation of the gravitational binding energy in compact binaries
• Monte-Carlo simulations of black hole mergers in AGN disks: Low ${\chi }_{\mathrm{eff}}$ mergers and predictions for LIGO
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
• Convolutional neural networks: a magic bullet for gravitational-wave detection?
• Bayesian analysis of LIGO-Virgo mergers: Primordial vs. astrophysical black hole populations
• Searching for Eccentricity: Signatures of Dynamical Formation in the First Gravitational-Wave Transient Catalogue of LIGO and Virgo
• Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
• Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
• The GW190521 Mass Gap Event and the Primordial Black Hole Scenario
• Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
• Characterization of systematic error in Advanced LIGO calibration
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• Binary black holes in young star clusters: the impact of metallicity
• Testing gravity with cold atom interferometry: Results and prospects
• Mass-gap Mergers in Active Galactic Nuclei
• The properties of merging black holes and neutron stars across cosmic time
• Nested Sampling with Normalising Flows for Gravitational-Wave Inference
• Black hole mergers from quadruples
• The Evolution of Primordial Black Holes and their Final Observable Spins
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Binary black holes in the pair-instability mass gap
• Learning Bayesian posteriors with neural networks for gravitational-wave inference
• Improved gravitational-wave constraints on higher-order curvature theories of gravity
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach I: Regularized Lagrangian
• Conservative Tidal Effects in Compact Binary Systems to Next-to-Leading Post-Minkowskian Order
• Non-linear dynamics of spinning bosonic stars: formation and stability
• Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• Eccentric Black Hole Mergers in Active Galactic Nuclei
• Testing the black-hole area law with GW150914
• Phase effects from strong gravitational lensing of gravitational waves
• From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch
• Tests of General Relativity with GWTC-3
• Machine-learning non-stationary noise out of gravitational wave detectors
• Implications of Eccentric Observations on Binary Black Hole Formation Channels
• GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
• Orbital Evolution of Equal-mass Eccentric Binaries due to a Gas Disk: Eccentric Inspirals and Circular Outspirals
• The Science Case for LIGO-India
• Searches for Continuous-Wave Gravitational Radiation
• Distance measures in gravitational-wave astrophysics and cosmology
• Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case
• Primordial black holes and secondary gravitational waves from k/G inflation
• Spin Evolution of Stellar-mass Black Hole Binaries in Active Galactic Nuclei
• Constraints on the astrophysical environment of binaries with gravitational-wave observations
• Strong gravitational lensing and shadow constraint from M87* of slowly rotating Kerr-like black hole
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• Close Binary Companions to APOGEE DR16 Stars: 20,000 Binary-star Systems Across the Color-Magnitude Diagram
• EHT constraint on the ultralight scalar hair of the M87 supermassive black hole
• Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs
• Characterization of the stochastic signal originating from compact binaries populations as measured by LISA
• Gauge Independence of Induced Gravitational Waves
• Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
• Short GRB Host Galaxies I: Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets
• Ringdown overtones, black hole spectroscopy, and no-hair theorem tests
• ELGAR -- a European Laboratory for Gravitation and Atom-interferometric Research
• Black hole genealogy: Identifying hierarchical mergers with gravitational waves
• Gravitational waves induced from primordial black hole fluctuations: The effect of an extended mass function
• Constraining the masses of microlensing black holes and the mass gap with Gaia DR2
• Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals
• Extending the PyCBC search for gravitational waves from compact binary mergers to a global network
• Neutron Star Merger Remnants
• Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's first observing run
• Anatomy of single-field inflationary models for primordial black holes
• Distinguishing Primordial Black Holes from Astrophysical Black Holes by Einstein Telescope and Cosmic Explorer
• Spontaneous scalarization
• Constraining a modified gravity theory in strong gravitational lensing and black hole shadow observations
• Minding the gap: GW190521 as a straddling binary
• Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning
• The Clustering Evolution of Primordial Black Holes
• Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically
• The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky
• Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution
• Evidence for primordial black hole dark matter from LIGO/Virgo merger rates
• Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
• An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Constraining the equation of state of high-density cold matter using nuclear and astronomical measurements
• On the maximum mass of neutron stars and GW190814
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity
• GW190521 may be an intermediate mass ratio inspiral
• Measuring the star formation rate with gravitational waves from binary black holes
• Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
• New twists in compact binary waveform modelling: a fast time domain model for precession
• Amorphous optical coatings of present gravitational-wave interferometers
• Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
• Distribution of Effective Spins and Masses of Binary Black Holes from the LIGO and Virgo O1-O3a Observing Runs
• Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
• Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries
• Probing Fundamental Physics with Gravitational Waves: The Next Generation
• Constraints on quasi-normal-mode frequencies with LIGO-Virgo binary-black-hole observations
• Measuring the dark matter environments of black hole binaries with gravitational waves
• Low-Latency Gravitational Wave Alerts for Multi-Messenger Astronomy During the Second Advanced LIGO and Virgo Observing Run
• Dynamical descalarization in binary black hole mergers
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries
• Primordial Black Hole Dark Matter and the LIGO/Virgo observations
• Reducing Scattered Light in LIGO's Third Observing Run
• Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH
• Repeated mergers and ejection of black holes within nuclear star clusters
• On the Origin of GW190521-like events from repeated black hole mergers in star clusters
• Numerical relativity simulation of GW150914 beyond general relativity
• Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
• Revising natal kick prescriptions in population synthesis simulations
• Gravitational Wave Denoising of Binary Black Hole Mergers with Deep Learning
• The Gravitational-Wave Physics II: Progress
• GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger
• Superradiance in String Theory
• Stellar-mass black holes in young massive and open stellar clusters IV: updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data
• Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)
• Intermediate Mass Black Hole Formation in compact Young Massive Star Clusters
• Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes
• Black hole superradiant instability from ultralight spin-2 fields
• Fast evaluation of multi-detector consistency for real-time gravitational wave searches
• Gravitational wave signatures of ultralight vector bosons from black hole superradiance
• Ultra-slow-roll inflation with quantum diffusion
• Merger rate density of Population III binary black holes below, above, and in the pair-instability mass gap
• Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
• kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
• On the properties of the massive binary black hole merger GW170729
• Dissecting the growth of the power spectrum for primordial black holes
• The shadows and observational appearance of a noncommutative black hole surrounded by various profiles of accretions
• Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
• Advanced LIGO detector performance in the fourth observing run
• Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies
• Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals
• All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data
• Frequency-Dependent Squeezed Vacuum Source for Broadband Quantum Noise Reduction in Advanced Gravitational-Wave Detectors
• The Low Effective Spin of Binary Black Holes and Implications for Individual Gravitational-Wave Events
• Constraining the abundance of primordial black holes with gravitational lensing of gravitational waves at LIGO frequencies
• Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics
• Fingerprints of binary black hole formation channels encoded in the mass and spin of merger remnants
• Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis
• The most ordinary formation of the most unusual double black hole merger
• Science with the TianQin Observatory: Preliminary Results on Stochastic Gravitational-Wave Background
• GW250114: testing Hawking's area law and the Kerr nature of black holes
• Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes
• From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back)
• Thanks for the memory: measuring gravitational-wave memory in the first LIGO/Virgo gravitational-wave transient catalog
• Is GW190521 the merger of black holes from the first stellar generations?
• Gravitational-wave constraints on the equatorial ellipticity of millisecond pulsars
• Gravitational wave probes of dark matter: challenges and opportunities
• AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state
• Constraining the orbital eccentricity of inspiralling compact binary systems with Advanced LIGO
• Orbital evolution of binary black holes in active galactic nucleus disks: a disk channel for binary black hole mergers?
• Shouts and Murmurs: Combining Individual Gravitational-Wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers
• Scalar induced gravitational waves in inflation with gravitationally enhanced friction
• Omicron: a tool to characterize transient noise in gravitational-wave detectors
• Conservative and radiative dynamics of spinning bodies at third post-Minkowskian order using worldline quantum field theory
• GRANDMA Observations of Advanced LIGO's and Advanced Virgo's Third Observational Campaign
• Distinguishing fuzzballs from black holes through their multipolar structure
• Lunar Gravitational-Wave Antenna
• All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
• Direct limits for scalar field dark matter from a gravitational-wave detector
• The Science of the Einstein Telescope
• Detecting Gravitational Waves With Disparate Detector Responses: Two New Binary Black Hole Mergers
• Realtime search for compact binary mergers in Advanced LIGO and Virgo's third observing run using PyCBC Live
• Follow-up of the Neutron Star Bearing Gravitational Wave Candidate Events S190425z and S190426c with MMT and SOAR
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Black-hole spectroscopy, the no-hair theorem and GW150914: Kerr vs. Occam
• Parameter estimation with gravitational waves
• Black Hole Coagulation: Modeling Hierarchical Mergers in Black Hole Populations
• Constraints on ultralight scalar bosons within black hole spin measurements from LIGO-Virgo's GWTC-2
• Effective-one-body waveforms for precessing coalescing compact binaries with post-newtonian Twist
• Constraints on Primordial Black Holes: the Importance of Accretion
• 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
• Potential gravitational-wave signatures of quantum gravity
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• Pulsar Timing Array Constraints on the Induced Gravitational Waves
• Spectroscopy of binary black hole ringdown using overtones and angular modes
• Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
• Stability of rotating scalar boson stars with nonlinear interactions
• The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach: potential contributions
• Constraints on Stupendously Large Black Holes
• Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity
• Gravitational-wave physics with Cosmic Explorer: limits to low-frequency sensitivity
• The Most Massive Binary Black Hole Detections and the Identification of Population Outliers
• Universal Properties of Light Rings for Stationary Axisymmetric Spacetimes
• Gravitational waves from bubble collisions and fluid motion in strongly supercooled phase transitions
• Detectability of Intermediate-Mass Black Holes in Multiband Gravitational Wave Astronomy
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• Black Hole Mergers from Hierarchical Triples in Dense Star Clusters
• Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
• Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
• Fourth post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
• Realistic sensitivity curves for pulsar timing arrays
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• The Emergence of Structure in the Binary Black Hole Mass Distribution
• Black hole-neutron star mergers from triples
• Are stellar-mass black-hole binaries too quiet for LISA?
• Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2
• Inferring the properties of a population of compact binaries in presence of selection effects
• Search for ultralight bosons in Cygnus X-1 with Advanced LIGO
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Probing multiple populations of compact binaries with third-generation gravitational-wave detectors
• Primordial Black Holes from Supercooled Phase Transitions
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
• No massive black holes in the Milky Way halo
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Primordial black hole tower: Dark matter, earth-mass, and LIGO black holes
• Static spherical vacuum solutions in the bumblebee gravity model
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
• Radiation-reaction force and multipolar waveforms for eccentric, spin-aligned binaries in the effective-one-body formalism
• Constraints on Einstein-dilaton-Gauss-Bonnet gravity from Black Hole-Neutron Star Gravitational Wave Events
• Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• Primordial black holes and secondary gravitational waves from inflationary model with a non-canonical kinetic term
• Identifying strong gravitational-wave lensing during the second observing run of Advanced LIGO and Advanced Virgo
• Gravitational wave signal recognition of O1 data by deep learning
• Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field
• Dynamics of black hole - neutron star binaries in young star clusters
• Enabling real-time multi-messenger astrophysics discoveries with deep learning
• Noise Reduction in Gravitational-wave Data via Deep Learning
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• Gravitational wave lensing beyond general relativity: birefringence, echoes and shadows
• Overtones or higher harmonics? Prospects for testing the no-hair theorem with gravitational wave detections
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• Constraining cosmological phase transitions with the Parkes Pulsar Timing Array
• Ringing of rotating black holes in higher-derivative gravity
• Searching for a Ringdown Overtone in GW150914
• Black Hole Binary Formation in AGN Discs: From Isolation to Merger
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
• Non-tensorial Gravitational Wave Background in NANOGrav 12.5-Year Data Set
• When are LIGO/Virgo's Big Black-Hole Mergers?
• A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism
• The mass gap, the spin gap, and the origin of merging binary black holes
• PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
• Primordial black hole merger rates: distributions for multiple LIGO observables
• Gravitational Lensing of Gravitational Waves: Effect of Microlens Population in Lensing Galaxies
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Quasinormal-mode filters: a new approach to analyze the gravitational-wave ringdown of binary black-hole mergers
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Heterodyned Likelihood for Rapid Gravitational Wave Parameter Inference
• Search for strongly lensed counterpart images of binary black hole mergers in the first two LIGO observing runs
• Black Hole Formation in the Lower Mass Gap through Mergers and Accretion in AGN Disks
• A detailed analysis of GW190521 with phenomenological waveform models
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
• Black-hole ringdown as a probe of higher-curvature gravity theories
• Neutrino transport in general relativistic neutron star merger simulations
• On the origin of GW190425
• Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers
• Discovering features in gravitational-wave data through detector characterization, citizen science and machine learning
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms
• Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order
• Search for Eccentric Binary Neutron Star Mergers in the first and second observing runs of Advanced LIGO
• Detecting Double Neutron Stars with LISA
• The universal Teukolsky equations and black hole perturbations in higher-derivative gravity
• Testing the nature of gravitational-wave polarizations using strongly lensed signals
• The next decade of black hole spectroscopy
• The peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA
• Constraining the neutron star equation of state using multi-band independent measurements of radii and tidal deformabilities
• No signature of the orbital motion of a putative 70 solar mass black hole in LB-1
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• Looking at the NANOGrav Signal Through the Anthropic Window of Axion-Like Particles
• Outlook for detecting the gravitational wave displacement and spin memory effects with current and future gravitational wave detectors
• Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
• Chemically Homogeneous Evolution: A rapid population synthesis approach
• The binary black hole spin distribution likely broadens with redshift
• Subtracting glitches from gravitational-wave detector data during the third observing run
• Binary Black Hole Merger Rates in AGN Disks versus Nuclear Star Clusters: Loud beats Quiet
• Accelerating parameter estimation of gravitational waves from compact binary coalescence using adaptive frequency resolutions
• Binary Black Hole Mergers from LIGO/Virgo O1 and O2: Population Inference Combining Confident and Marginal Events
• Jumping the gap: searching for LIGO's biggest black holes
• Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data
• Detecting Gravitational Waves in Data with Non-Gaussian Noise
• Bridging the Gap: Categorizing Gravitational-Wave Events at the Transition Between Neutron Stars and Black Holes
• The implications of high BH spins on the origin of BH-BH mergers
• Gravitational-Wave Constraints on an Effective Field-Theory Extension of General Relativity
• Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• Exploring Features in the Binary Black Hole Population
• Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Environmental Noise in Advanced LIGO Detectors
• Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
• Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: Gravitational Wave Bursts and Electromagnetic Counterparts from Merging Stellar Black Hole Binaries
• Peaks and primordial black holes: the effect of non-Gaussianity
• Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• $\text{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors
• How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?
• Detection of gravitational-wave signals from binary neutron star mergers using machine learning
• Spitzer Observations of the Predicted Eddington Flare from Blazar OJ 287
• Scalar perturbations around rotating regular black holes and wormholes: quasi-normal modes, ergoregion instability and superradiance
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Prospects for probing gravitational waves from primordial black hole binaries
• 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
• Accelerated, Scalable and Reproducible AI-driven Gravitational Wave Detection
• Multi-messenger observations of binary neutron star mergers in the O4 run
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Coalescence of black hole--neutron star binaries
• Importance of mirror modes in binary black hole ringdown waveform
• Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity
• Black Hole and Neutron Star Binary Mergers in Triple Systems: II. Merger Eccentricity and Spin-Orbit Misalignment
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• The landscape of disk outflows from black hole - neutron star mergers
• A Parameter-Free Tour of the Binary Black Hole Population
• Merging Black Holes in the Low-mass and High-mass Gaps from 2+2 Quadruple Systems
• Populations of stellar mass Black holes from binary systems
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• A generalized precession parameter ${\chi }_{\mathrm{p}}$ to interpret gravitational-wave data
• Small-scale structure of primordial black hole dark matter and its implications for accretion
• Mass-redshift Degeneracy for Gravitational-wave Sources in the Vicinity of a Supermassive Black Hole
• Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
• Polarizations of Gravitational Waves in the Bumblebee Gravity Model
• Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
• Parameterized and inspiral-merger-ringdown consistency tests of gravity with multi-band gravitational wave observations
• Self-Force Calculations with a Spinning Secondary
• An approach to computing spectral shifts for black holes beyond Kerr
• Two-harmonic approximation for gravitational waveforms from precessing binaries
• Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI
• Perturbing the perturbed: Stability of quasinormal modes in presence of a positive cosmological constant
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• Gravitational spin-orbit coupling through third-subleading post-Newtonian order: from first-order self-force to arbitrary mass ratios
• General relativistic simulations of the quasi-circular inspiral and merger of charged black holes: GW150914 and fundamental physics implications
• Asteroids for $\mu$Hz gravitational-wave detection
• Luminous Red Novae: population models and future prospects
• POEMMA's Target of Opportunity Sensitivity to Cosmic Neutrino Transient Sources
• Searching for Dark Photon Dark Matter in LIGO O1 Data
• Low mechanical loss TiO${}_2$:GeO${}_2$ coatings for reduced thermal noise in Gravitational Wave Interferometers
• Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
• Constraining gravitational wave amplitude birefringence and Chern-Simons gravity with GWTC-2
• Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• On the possibility of GW190425 being a black hole--neutron star binary merger
• Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+0451 data
• Identifying Type II Strongly Lensed Gravitational-Wave Images in Third-Generation Gravitational-Wave Detectors
• Extracting the Gravitational Recoil from Black Hole Merger Signals
• GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
• A fast and precise methodology to search for and analyse strongly lensed gravitational-wave events
• Cylindrical Systems in General Relativity
• Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• MLGWSC-1: The first Machine Learning Gravitational-Wave Search Mock Data Challenge
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• The last migration trap of compact objects in AGN accretion disc
• No evidence that the majority of black holes in binaries have zero spin
• Linear Response, Hamiltonian and Radiative Spinning Two-Body Dynamics
• Ain't No Mountain High Enough: Semi-Parametric Modeling of LIGO-Virgos Binary Black Hole Mass Distribution
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
• Constraining black hole mimickers with gravitational wave observations
• Multiparameter tests of general relativity using multiband gravitational-wave observations
• Neutron Star Mergers in AGN Accretion Disks: Cocoon and Ejecta Shock Breakouts
• Merger rate density of binary black holes formed in open clusters
• The merger history of primordial-black-hole binaries
• Single-single gravitational-wave captures in globular clusters: Eccentric deci-Hertz sources observable by DECIGO and Tian-Qin
• Role of black hole quasinormal mode overtones for ringdown analysis
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Dependence of Gravitational Wave Transient Rates on Cosmic Star Formation and Metallicity Evolution History
• Constraints on compact dark matter from gravitational wave microlensing
• Binary radial velocity measurements with space-based gravitational-wave detectors
• Resolving the Stellar-Collapse and Hierarchical-Merger origins of the Coalescing Black Holes
• Primordial Gravitational Wave Signals in Modified Cosmologies
• Search for the Gravitational-wave Background from Cosmic Strings with the Parkes Pulsar Timing Array Second Data Release
• Hereditary Terms at Next-To-Leading Order in Two-Body Gravitational Dynamics
• Unbiased Hubble constant estimation from binary neutron star mergers
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• Joint gravitational wave -- gamma-ray burst detection rates in the aftermath of GW170817
• Probing planetary-mass primordial black holes with continuous gravitational waves
• Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM
• Deep learning for multimessenger core-collapse supernova detection
• A Systematic View of Ten New Black Hole Spins
• Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties
• PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• GW190412 as a Third-Generation Black Hole Merger from a Super Star Cluster
• Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation
• Learning about black hole binaries from their ringdown spectra
• Search for continuous gravitational waves from 20 accreting millisecond X-ray pulsars in O3 LIGO data
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• GPU-accelerated massive black hole binary parameter estimation with LISA
• Black hole mergers of AGN origin in LIGO/Virgo's O1-O3a observing periods
• LIGO Detector Characterization in the first half of the fourth Observing run
• Rapid Parameter Estimation of Gravitational Waves from Binary Neutron Star Coalescence using Focused Reduced Order Quadrature
• Primordial black holes and secondary gravitational waves from natural inflation
• Virgo Detector Characterization and Data Quality: results from the O3 run
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• Source of black bounces in general relativity
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• The Memory Remains (Undetected): Updates from the Second LIGO/Virgo Gravitational-Wave Transient Catalog
• A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model
• Chirp Mass and Spin of Binary Black Holes from First Star Remnants
• Spin-induced dynamical scalarization, de-scalarization and stealthness in scalar-Gauss-Bonnet gravity during black hole coalescence
• Gravitational spin-orbit and aligned spin${}_1$-spin${}_2$ couplings through third-subleading post-Newtonian orders
• Kilonova Detectability with Wide-Field Instruments
• Lensing of gravitational waves as a probe of compact dark matter
• Initial clustering and the primordial black hole merger rate
• Waveform of gravitational waves in the ghost-free parity-violating gravities
• Machine Learning Gravitational Waves from Binary Black Hole Mergers
• Dark photon superradiance: Electrodynamics and multimessenger signals
• Uncertainty limits on neutron star radius measurements with gravitational waves
• How to assess the primordial origin of single gravitational-wave events with mass, spin, eccentricity, and deformability measurements
• You Can't Always Get What You Want: The Impact of Prior Assumptions on Interpreting GW190412
• Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• Hyperboloidal framework for the Kerr spacetime
• Primordial black hole formation during the QCD phase transition: threshold, mass distribution and abundance
• Black holes in the low mass gap: Implications for gravitational wave observations
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• A brief overview of black hole-neutron star mergers
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
• High rate of gravitational waves mergers from flyby perturbations of wide black-hole triples in the field
• Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission
• Instability of rotating Bose stars
• Black hole and neutron star mergers in Galactic Nuclei: the role of triples
• Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
• Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
• Re-estimating the Spin Parameter of the Black Hole in Cygnus X-1
• Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Primordial black hole formation by vacuum bubbles II
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• Gravitational lensing of gravitational waves: wave nature and prospects for detection
• Unified model for the LISA measurements and instrument simulations
• Shot noise in the astrophysical gravitational-wave background
• Stirred and shaken: dynamical behavior of boson stars and dark matter cores
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• Deep learning for clustering of continuous gravitational wave candidates
• Gaia May Detect Hundreds of Well-characterised Stellar Black Holes
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Constraints on the distance duality relation with standard sirens
• White dwarf binaries suggest a common envelope efficiency $\alpha \sim 1/3$
• Short gamma-ray bursts within 200 Mpc
• PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
• In-depth analysis of the clustering of dark matter particles around primordial black holes I: density profiles
• Tidal effects in the equations of motion of compact binary systems to next-to-next-to-leading post-Newtonian order
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Gaussian processes reconstruction of modified gravitational wave propagation
• The Role of Topological Photon Spheres in Constraining the Parameters of Black Holes
• 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
• SuperRad: Modeling the black hole superradiance gravitational waveform
• Repeated Gravitational Lensing of Gravitational Waves in Hierarchical Black Hole Triples
• Cosmologically coupled compact objects: a single parameter model for LIGO--Virgo mass and redshift distributions
• Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
• Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Breaking the mass-sheet degeneracy with gravitational wave interference in lensed events
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Status and perspectives of Continuous Gravitational Wave searches
• Primordial black holes and secondary gravitational waves from the Higgs field
• Assessing the impact of transient orbital resonances
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• Using rational filters to uncover the first ringdown overtone in GW150914
• The SXS Collaboration's third catalog of binary black hole simulations
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Coincident f(Q) gravity: black holes, regular black holes and black bounces
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Black hole spectroscopy by mode cleaning
• A new spin on LIGO-Virgo binary black holes
• Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
• High-overtone fits to numerical relativity ringdowns: beyond the dismissed n=8 special tone
• When will we observe binary black holes precessing?
• Gravitational wave constraints on Lorentz and parity violations in gravity: high-order spatial derivative cases
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Gravitational-wave versus X-ray tests of strong-field gravity
• Primordial black holes and gravitational waves from non-canonical inflation
• Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Microlensing optical depth and event rate toward the Large Magellanic Cloud based on 20 years of OGLE observations
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Eliminating the LIGO bounds on primordial black hole dark matter
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
• Search for nonlinear memory from subsolar mass compact binary mergers
• Gravitational-Wave Implications for the Parity Symmetry of Gravity at GeV Scale
• Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
• Gravitational axial perturbations of Schwarzschild-like black holes in dark matter halos
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• Constraints on the Nieh-Yan modified teleparallel gravity with gravitational waves
• Constraining the mass of the graviton with the planetary ephemeris INPOP
• Modelling the Ringdown from Precessing Black Hole Binaries
• A New Gravitational Wave Signature of Low-$T/|W|$ Instability in Rapidly Rotating Stellar Core Collapse
• Numerical simulation of sky localization for LISA-TAIJI joint observation
• Imprints of r-process heating on fall-back accretion: distinguishing black hole-neutron star from double neutron star mergers
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Rotating hairy black holes and thermodynamics from gravitational decoupling
• Gravitational-wave astronomy with a physical calibration model
• Dissipation in extreme-mass ratio binaries with a spinning secondary
• Teamwork Makes the Dream Work: Optimizing Multi-Telescope Observations of Gravitational-Wave Counterparts
• Assessing the data-analysis impact of LISA orbit approximations using a GPU-accelerated response model
• Bumblebee black holes in light of Event Horizon Telescope observations
• Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions
• Gravitational wave detectors with broadband high frequency sensitivity
• Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries
• Deep-Learning Continuous Gravitational Waves: Multiple detectors and realistic noise
• Primordial black holes from metric preheating: mass fraction in the excursion-set approach
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
• Constraints on the rotating self-dual black hole with quasi-periodic oscillations
• Lessons for adaptive mesh refinement in numerical relativity
• Constraining extra-spatial dimensions with observations of GW170817
• Gravitational scattering at the seventh order in $G$: nonlocal contribution at the sixth post-Newtonian accuracy
• Updated universal relations for tidal deformabilities of neutron stars from phenomenological equations of state
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Multi-band gravitational wave tests of general relativity
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• Testing General Relativity with Gravitational Waves: An Overview
• A Machine Learning Based Source Property Inference for Compact Binary Mergers
• The Origin of inequality: isolated formation of a 30+10Msun binary black-hole merger
• Measuring precession in asymmetric compact binaries
• A scalable random forest regressor for combining neutron-star equation of state measurements: A case study with GW170817 and GW190425
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case
• Point absorbers in Advanced LIGO
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• No Detectable Kilonova Counterpart is Expected for O3 Neutron Star-Black Hole Candidates
• Tidal response from scattering and the role of analytic continuation
• The sum of Love: Exploring the effective tidal deformability of neutron stars
• Inferring eccentricity evolution from observations of coalescing binary black holes
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Weighing in on black hole binaries with BPASS: LB-1 does not contain a 70M${}_{\odot }$ black hole
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Constraints on primordial black holes from LIGO-Virgo-KAGRA O3 events
• Multi-field, multi-frequency bosonic stars and a stabilization mechanism
• Constraints on primordial curvature spectrum from primordial black holes and scalar-induced gravitational waves
• Quantifying the Effect of Power Spectral Density Uncertainty on Gravitational-Wave Parameter Estimation for Compact Binary Sources
• Eccentric self-forced inspirals into a rotating black hole
• Search for a scalar induced stochastic gravitational wave background in the third LIGO-Virgo observing run
• Standard-siren cosmology using gravitational waves from binary black holes
• Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei
• Testing Gravity with Gravitational Waves from Binary Black Hole Mergers: Contributions from Amplitude Corrections
• An Experiment for Observing Quantum Gravity Phenomena using Twin Table-Top 3D Interferometers
• Gravity in the infrared and effective nonlocal models
• Targeted Sub-threshold Search for Strongly-lensed Gravitational-wave Events
• A New Spin on an Old Black Hole: NuSTAR Spectroscopy of EXO 1846-031
• Gravitational-Wave Lunar Observatory for Cosmology
• A Bayesian inference of relativistic mean-field model for neutron star matter from observation of NICER and GW170817/AT2017gfo
• Brans-Dicke theory in Bondi-Sachs form: Asymptotically flat solutions, asymptotic symmetries and gravitational-wave memory effects
• A trend in the effective spin distribution of LIGO binary black holes with mass
• Removing degeneracy and multimodality in gravitational wave source parameters
• Constraining the neutron-matter equation of state with gravitational waves
• Simultaneously probing the sound speed and equation of state of the early Universe with pulsar timing arrays
• Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A
• VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions
• Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
• The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-Up of Gravitational Wave Events
• Improved time-delay lens modelling and $H_0$ inference with transient sources
• Rapid Identification of Strongly Lensed Gravitational-Wave Events with Machine Learning
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• Primordial black holes and scalar-induced gravitational waves from the generalized Brans-Dicke theory
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data
• Adding eccentricity to quasicircular binary-black-hole waveform models
• IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
• Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches
• Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Detection Prospects of Core-Collapse Supernovae with Supernova-Optimized Third-Generation Gravitational-wave Detectors
• A search for optical and near-infrared counterparts of the compact binary merger GW190814
• A Rosetta Stone for eccentric gravitational waveform models
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Lensing or luck? False alarm probabilities for gravitational lensing of gravitational waves
• Search for gravitational waves from high-mass-ratio compact-binary mergers of stellar mass and sub-solar mass black holes
• Probing ultralight dark matter with future ground-based gravitational-wave detectors
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Constraining extra dimensions using observations of black hole quasi-normal modes
• Gravitational Wave Interference via Gravitational Lensing: Measurements of Luminosity Distance, Lens Mass, and Cosmological Parameters
• Tight constraints on Einstein-dilation-Gauss-Bonnet gravity from GW190412 and GW190814
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• (H)DPGMM: A Hierarchy of Dirichlet Process Gaussian Mixture Models for the inference of the black hole mass function
• Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
• Systematic bias on the inspiral-merger-ringdown consistency test due to neglect of orbital eccentricity
• Eccentric binary black hole mergers in globular clusters hosting intermediate-mass black holes
• Gravitational-wave memory effects in Brans-Dicke theory: Waveforms and effects in the post-Newtonian approximation
• First-order phase transition and fate of false vacuum remnants
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• The tune of the universe: the role of plasma in tests of strong-field gravity
• Binary black hole spectroscopy: a no-hair test of GW190814 and GW190412
• Extraction of Binary Black Hole Gravitational Wave Signals from Detector Data Using Deep Learning
• Quasinormal Modes of a Black Hole with Quadrupole Moment
• Impact of the wave-like nature of Proca stars on their gravitational-wave emission
• Eikonal quasinormal modes of black holes beyond general relativity III: scalar Gauss-Bonnet gravity
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• Directed search for continuous gravitational-wave signals from the Galactic Center in the Advanced LIGO second observing run
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Feedback-Dominated Accretion Flows
• Parameter estimation of stellar-mass black hole binaries with LISA
• Spin effects in gravitational waveforms and fluxes for binaries on eccentric orbits to the third post-Newtonian order
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• Constraining the Merger History of Primordial-Black-Hole Binaries from GWTC-3
• Application of dictionary learning to denoise LIGO's blip noise transients
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• Turn up the volume: Listening to phase transitions in hot dark sectors
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Flexible and Fast Estimation of Binary Merger Population Distributions with Adaptive KDE
• Compact object scalarization with general relativity as a cosmic attractor
• Gravitational wave population inference with deep flow-based generative network
• Frequency response of space-based interferometric gravitational-wave detectors
• Potential Subpopulations and Assembling Tendency of the Merging Black Holes
• Comparing Effective One Body Hamiltonians for spin-aligned coalescing binaries
• Effective spin distribution of black hole mergers in triples
• Identifying when Precession can be Measured in Gravitational Waveforms
• Deep Residual Networks for Gravitational Wave Detection
• Equatorial timelike circular orbits around generic ultracompact objects
• Gravitational-wave inference in the catalog era: evolving priors and marginal events
• Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation
• Gravitational waveforms from periodic orbits around a quantum-corrected black hole
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Rapid Black Hole Spin-down by Thick Magnetically Arrested Disks
• Phase shift of gravitational waves induced by aberration
• The onset of spontaneous scalarization in generalised scalar-tensor theories
• Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach
• Parametrized tests of post-Newtonian theory using principal component analysis
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Search for black hole hyperbolic encounters with gravitational wave detectors
• Built-in scordatura in U-DHOST
• Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
• Gravelamps: Gravitational Wave Lensing Mass Profile Model Selection
• Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
• Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
• Gravitational-wave luminosity distance in quantum gravity
• Black Hole Superradiance in the Presence of Lorentz Symmetry Violation
• Suppressing parametric instabilities in LIGO using low-noise acoustic mode dampers
• Limits on hierarchical black hole mergers from the most negative ${\chi }_{\mathrm{eff}}$ systems
• A Late-time Radio Survey of Short GRBs at $z<0.5$: New Constraints on the Remnants of Neutron Star Mergers
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• Search for gravitational-wave signals associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo
• Pre-merger localization of compact-binary mergers with third generation observatories
• Ultralight Fermionic Dark Matter
• Standard Sirens as a novel probe of dark energy
• Malaise and remedy of binary boson-star initial data
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• On mass distribution of coalescing black holes
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Recognizing black holes in gravitational-wave observations: Challenges in telling apart impostors in mass-gap binaries
• Exploring the NANOGrav Signal and Planet-mass Primordial Black Holes through Higgs Inflation
• Dynamical evolution of Population III stellar systems and the resulting binary statistics
• Extreme Gravity and Fundamental Physics
• Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
• Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
• Testing Theories of Gravity with Planetary Ephemerides
• New binary black hole mergers in the LIGO-Virgo O3b data
• Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors
• GW170817A as a Hierarchical Black Hole Merger
• Reconstruction of Primordial Power Spectrum of curvature perturbation from the merger rate of Primordial Black Hole Binaries
• Using Deep Learning to Localize Gravitational Wave Sources
• Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• Tail contributions to gravitational conservative dynamics
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Constraints on the phase transition and nuclear symmetry parameters from PSR $\mathrm{J}0740+6620$ and multimessenger data of other neutron stars
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• Gravitational Waves from Hierarchical Triple Systems with Kozai-Lidov Oscillation
• Impacts of overlapping gravitational-wave signals on the parameter estimation: Toward the search for cosmological backgrounds
• Adapting time-delay interferometry for LISA data in frequency
• Scattering of gravitational waves off spinning compact objects with an effective worldline theory
• Compact Michelson interferometers with subpicometer sensitivity
• Measuring binary black hole orbital-plane spin orientations
• Black hole spectroscopy horizons for current and future gravitational wave detectors
• Black hole spins in coalescing binary black holes
• Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission
• Probing the speed of scalar-induced gravitational waves with pulsar timing arrays
• Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
• Assessing the model waveform accuracy of gravitational waves
• On modeling for Kerr black holes: Basis learning, QNM frequencies, and spherical-spheroidal mixing coefficients
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3a
• Improved constraints from ultra-faint dwarf galaxies on primordial black holes as dark matter
• On the classification of Generalized Quasitopological Gravities
• Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• Gas Assisted Binary Black Hole Formation in AGN Discs
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• Serendipitous Discoveries of Kilonovae in the LSST Main Survey: Maximising Detections of Sub-Threshold Gravitational Wave Events
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Evolution of Retrograde Orbiters in an AGN Disk
• Detecting the Beaming Effect of Gravitational Waves
• Deflection angle of a light ray reflected by a general marginally unstable photon sphere in a strong deflection limit
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Detectability of the subdominant mode in a binary black hole ringdown
• The Interplay between the Dark Matter Axion and Primordial Black Holes
• Improved deep learning techniques in gravitational-wave data analysis
• Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• A Higher Probability of Detecting Lensed Supermassive Black Hole Binaries by LISA
• Ruling out Initially Clustered Primordial Black Holes as Dark Matter
• Gravitational wave memory beyond general relativity
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• On Black Hole Temperature in Horndeski Gravity
• Analytic Kludge Waveforms for Extreme Mass Ratio Inspirals of Charged Object around Kerr-Newman Black Hole
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Imprints of dark matter on gravitational ringing of supermassive black holes
• Spectral method for metric perturbations of black holes: Kerr background case in general relativity
• High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• Improved statistic to identify strongly lensed gravitational wave events
• Early warning of coalescing neutron-star and neutron-star-black-hole binaries from nonstationary noise background using neural networks
• Signatures of ultralight bosons in the orbital eccentricity of binary black holes
• News from horizons in binary black hole mergers
• Improving the background of gravitational-wave searches for core collapse supernovae: A machine learning approach
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Search for the birefringence of gravitational waves with the third observing run of Advanced LIGO-Virgo
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• Characterisation of lensing selection effects for LISA massive black hole binary mergers
• Nonlogarithmic divergence of a deflection angle by a marginally unstable photon sphere of the Damour-Solodukhin wormhole in a strong deflection limit
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• Event rate predictions of strongly lensed gravitational waves with detector networks and more realistic templates
• Utilizing aLIGO Glitch Classifications to Validate Gravitational-Wave Candidates
• Archival searches for stellar-mass binary black holes in LISA
• Constraints on the ultralight scalar boson from Advanced LIGO and Advanced Virgo's first three observing runs using the stochastic gravitational-wave background
• Multi-waveform inference of gravitational waves
• A Late-Time Galaxy-Targeted Search for the Radio Counterpart of GW190814
• Forecasts on the speed of gravitational waves at high $z$
• Primordial Black Holes from CDM Isocurvature Perturbations
• Angular emission patterns of remnant black holes
• Gravitational wave observations, distance measurement uncertainties, and cosmology
• Formation threshold of rotating primordial black holes
• Searching for anisotropy in the distribution of binary black hole mergers
• Impact of a Spinning Supermassive Black Hole on the Orbit and Gravitational Waves of a Nearby Compact Binary
• Probing beyond-Kerr spacetimes with inspiral-ringdown corrections to gravitational waves
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Black Hole Hunting with LISA
• Probing Einstein-dilaton Gauss-Bonnet Gravity with the inspiral and ringdown of gravitational waves
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• Spectral Method for the Gravitational Perturbations of Black Holes: Schwarzschild Background Case
• Complete analysis of the background and anisotropies of scalar-induced gravitational waves: primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$ considered
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• New limits on the Lorentz/CPT symmetry through fifty gravitational-wave events
• Ringing of a black hole in a dark matter halo
• Gravitational-wave selection effects using neural-network classifiers
• Neutron Star-Black Hole Mergers from Gravitational Wave Captures
• From One to Many: A Deep Learning Coincident Gravitational-Wave Search
• Correlations in gravitational-wave reconstructions from eccentric binaries: A case study with GW151226 and GW170608
• All-sky, all-frequency directional search for persistent gravitational-waves from Advanced LIGO's and Advanced Virgo's first three observing runs
• Gravitational-wave constraints on the GWTC-2 events by measuring the tidal deformability and the spin-induced quadrupole moment
• The Importance of Priors on LIGO-Virgo Parameter Estimation: the Case of Primordial Black Holes
• LISA and the Existence of a Fast-Merging Double Neutron Star Formation Channel
• Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• Search for Continuous Gravitational Waves from the Central Compact Objects in Supernova Remnants Cassiopeia A, Vela Jr. and G347.3-0.5
• Black hole superradiant instability for massive spin-2 fields
• Tidal Spin-up of Black Hole Progenitor Stars
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Quantum Effects in Gravity Waves
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• Formation of mass gap objects in highly asymmetric mergers
• Tidal deformations of hybrid stars with sharp phase transitions and elastic crusts
• Revisiting the evidence for precession in GW200129 with machine learning noise mitigation
• Black-hole mergers in disklike environments could explain the observed $q$-${\chi }_{\mathrm{eff}}$ correlation
• Quasinormal Modes from EFT of Black Hole Perturbations with Timelike Scalar Profile
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Polarization distortions of lensed gravitational waves
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Cosmography using strongly lensed gravitational waves from binary black holes
• Evolution of massive stellar triples and implications for compact object binary formation
• Enhanced Curvature Perturbation and Primordial Black Hole Formation in Two-stage Inflation with a break
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• Theory-agnostic Reconstruction of Potential and Couplings from Quasi-Normal Modes
• Multi-messenger-Athena Synergy White Paper
• Numerical-relativity simulations of the quasi-circular inspiral and merger of non-spinning, charged black holes: methods and comparison with approximate approaches
• Probing the Black Hole Metric. I. Black Hole Shadows and Binary Black-Hole Inspirals
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events
• Consequences of neutron decay inside neutron stars
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Dark matter component in hadronic models with short-range correlations
• Algorithm for TDI numerical simulation and sensitivity investigation
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Probing Extremal Gravitational-Wave Events with Coarse-Grained Likelihoods
• Constraining the lensing of binary black holes from their stochastic background
• Gauge transformation of scalar induced gravitational waves
• Faint objects in motion: the new frontier of high precision astrometry
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Hyperbolic orbits on a cone
• Can a negative-mass cosmology explain dark matter and dark energy?
• Numerical investigation of plasma-driven superradiant instabilities
• Reconstructing gravitational wave signals from binary black hole mergers with minimal assumptions
• Cavity Detection of Gravitational Waves: Where Do We Stand?
• Testing general relativity using binary extreme-mass-ratio inspirals
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• Multimessenger parameter estimation of GW170817: from jet structure to the Hubble constant
• Tests of CPT invariance in gravitational waves with LIGO-Virgo catalog GWTC-1
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Ringdown frequencies in black holes formed from precessing black-hole binaries
• Tidal heating of Quantum Black Holes and their imprints on gravitational waves
• Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
• Nonlocal gravity and gravitational-wave observations
• Kicking gravitational wave detectors with recoiling black holes
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Inferring the gravitational wave memory for binary coalescence events
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• NANOGrav hints for first-order confinement-deconfinement phase transition in different QCD-matter scenarios
• Exploring strong-field deviations from general relativity via gravitational waves
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• Compact binary coalescences: Constraints on waveforms
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
• Time delay interferometry without clock synchronisation
• The Effect of Jet-Ejecta Interaction on the Viewing Angle Dependence of Kilonova Light Curves
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
• First gravitational-wave search for intermediate-mass black hole mergers with higher order harmonics
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• Regression methods in waveform modeling: a comparative study
• Black Hole Leftovers: The Remnant Population from Binary Black Hole Mergers
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• Electroweak Phase Transition and Gravitational Waves in the Type-II Seesaw Model
• Mass ejection in failed supernovae: equation of state and neutrino loss dependence
• First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure
• Inferring the maximum and minimum mass of merging neutron stars with gravitational waves
• 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
• Testing massive-field modifications of gravity via gravitational waves
• Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model
• Solving the Teukolsky equation with physics-informed neural networks
• Ready-to-use analytic model for gravitational waves from a hierarchical triple with Kozai-Lidov oscillations
• General relativistic simulations of collapsing binary neutron star mergers with Monte-Carlo neutrino transport
• Gauge transformation of scalar induced tensor perturbation during matter domination
• Filling the Mass Gap: How Kilonova Observations can Unveil the Nature of the Compact Object Merging with the Neutron Star
• Finding binary black holes in the Milky Way with LISA
• Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
• Lensing of Gravitational Waves as a Novel Probe of Graviton Mass
• Stars stripped in binaries -- the living gravitational wave sources
• Quasinormal modes in the field of a dyon-like dilatonic black hole
• Demographics of neutron stars in young massive and open clusters
• A bound on energy extraction (and hairiness) from superradiance
• Binary Neutron Stars Gravitational Wave Detection Based on Wavelet Packet Analysis And Convolutional Neural Networks
• An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
• Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black hole in a galactic nucleus
• Laser Frequency Noise in Next Generation Gravitational-Wave Detectors
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Optimization of model independent gravitational wave search using machine learning
• Observing an intermediate mass black hole GW190521 with minimal assumptions
• Generalized Approach to Matched Filtering using Neural Networks
• Anomaly Detection in Gravitational Waves data using Convolutional AutoEncoders
• Rapid and Robust Parameter Inference for Binary Mergers
• How loud are echoes from exotic compact objects?
• Investigating the relation between gravitational wave tests of general relativity
• Generalized disformal coupling leads to spontaneous tensorization
• Spherically symmetric static black holes in Einstein-aether theory
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Model independent tests of the Kerr bound with extreme mass ratio inspirals
• Pulsar timing array signals induced by black hole binaries in relativistic eccentric orbits
• Effective Potential and Topological Photon Spheres: A Novel Approach to Black Hole Parameter Classification
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Igniting weak interactions in neutron star postmerger accretion disks
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Bardeen solution with a cloud of strings
• The hydrodynamic evolution of binary black holes embedded within the vertically stratified disks of active galactic nuclei
• Comparing Remnant Properties from Horizon Data and Asymptotic Data in Numerical Relativity
• Constraining modifications of black hole perturbation potentials near the light ring with quasinormal modes
• Detecting the gravitational wave memory effect with TianQin
• Resolving Galactic binaries using a network of space-borne gravitational wave detectors
• Numerical simulations of stochastic inflation using importance sampling
• Transient gravitational waves from pulsar post-glitch recoveries
• Gravitational memory effects in Chern-Simons modified gravity
• Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
• Primordial Black Holes from Thermal Inflation
• Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study
• Lensing efficiency for gravitational wave mergers
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Doppler boosting the stochastic gravitational wave background
• Primordial black hole formation for an anisotropic perfect fluid: Initial conditions and estimation of the threshold
• Full analytical formulas for frequency response of space-based gravitational wave detectors
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• Null and time-like geodesics in Kerr-Newman black hole exterior
• Dynamics and Observational Signatures of Shell-like Black Hole Mimickers
• Signatures of primordial black holes in gravitational wave clustering
• Self-intersecting marginally outer trapped surfaces
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• Ensemble of Deep Convolutional Neural Networks for real-time gravitational wave signal recognition
• Heavy primordial black holes from strongly clustered light black holes
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• The impact of primordial binary on the dynamical evolution of intermediate massive star clusters
• AT2018kzr: the merger of an oxygen-neon white dwarf and a neutron star or black hole
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Identification and removal of non-Gaussian noise transients for gravitational wave searches
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Head-on collisions of $\ell$-boson stars
• A possible mass distribution of primordial black holes implied by LIGO-Virgo
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Implications for primordial black holes from cosmological constraints on scalar-induced gravitational wave
• Observing gravitational wave polarizations with LISA-TAIJI network
• Gravity Gradient Noise from Asteroids
• Neutrino spin oscillations in external fields in curved spacetime
• 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
• Gravitational-wave population inference at past time infinity
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Testing the"no-hair" nature of binary black holes using the consistency of multipolar gravitational radiation
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Fiducial displacements with improved accuracy for the global network of gravitational wave detectors
• Search for gravitational waves from twelve young supernova remnants with a hidden Markov model in Advanced LIGO's second observing run
• Solar mass black holes from neutron stars and bosonic dark matter
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Toward the primordial black hole formation threshold in a time-dependent equation-of-state background
• $r$-process nucleosynthesis from compact binary mergers
• Investigating tidal heating in neutron stars via gravitational Raman scattering
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Exploration of co-sputtered Ta${}_2$O${}_5$-ZrO${}_2$ thin films for gravitational-wave detectors
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Not quite black holes at LIGO
• Three-Body Effective Potential in General Relativity at Second Post-Minkowskian Order and Resulting Post-Newtonian Contributions
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Constraining Fundamental Physics with the Event Horizon Telescope
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
• Gravitational waves from mountains in newly born millisecond magnetars
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Optical Emission Model for Binary Black Hole Merger Remnants Travelling through Discs of Active Galactic Nuclei
• Sky localization of space-based gravitational wave detectors
• The connection between merging double compact objects and the Ultraluminous X-ray Sources
• Stable mass transfer can explain massive binary black hole mergers with a high spin component
• Eikonal quasinormal modes and photon orbits of deformed Schwarzschild black holes
• Constraining galactic structures of mirror dark matter
• Searches for Compact Binary Coalescence Events using Neural Networks in LIGO/Virgo Second Observation Period
• Characterizing the observation bias in gravitational-wave detections and finding structured population properties
• Efficient multi-timescale dynamics of precessing black-hole binaries
• Exploring non-singular black holes in gravitational perturbations
• Scalar-tensor mixed polarization search of gravitational waves
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• High Tide: A Systematic Search for Ellipsoidal Variables in ASAS-SN
• Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Jet Launching from Merging Magnetized Binary Neutron Stars with Realistic Equations of State
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number Counts
• Constraints on the electromagnetic counterpart of the Neutron Star Black Hole merger GW200115
• GWSkyNet: a real-time classifier for public gravitational-wave candidates
• Merging Compact Binaries Near a Rotating Supermassive Black Hole: Eccentricity Excitation due to Apsidal Precession Resonance
• An autoencoder neural network integrated into gravitational-wave burst searches to improve the rejection of noise transients
• High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap
• Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• NIR Counterparts to ULXs (III): Completing the photometric survey and selected spectroscopic results
• Ultimate fate of apparent horizons during a binary black hole merger II: Horizons weaving back and forth in time
• Binary intermediate-mass black hole mergers in globular clusters
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• Frequency response of time-delay interferometry for space-based gravitational wave antennas
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• Geometric approach for the modified second generation time delay interferometry
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than $\sim 20M_{\odot }$
• Extreme mass ratio inspirals in galaxies with dark matter halos
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Simulating Transient Noise Bursts in LIGO with Generative Adversarial Networks
• Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
• Measuring Individual Masses of Binary White Dwarfs with Space-based Gravitational-wave Interferometers
• Black Hole Ringdown as a Probe for Dark Energy
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• Echoes from braneworld wormholes
• Charged Black Hole Mergers: Orbit Circularisation and Chirp Mass Bias
• Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
• Upgraded antennas for pulsar observations in the Argentine Institute of Radio astronomy
• Combining Post-Circular and Padé approximations to compute Fourier domain templates for eccentric inspirals
• Inference of the neutron star equation of state from cosmological distances
• Unveiling the spectrum of inspiralling binary black holes
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Triaxially-deformed Freely-precessing Neutron Stars: Continuous electromagnetic and gravitational radiation
• Echoes from a singularity
• Gravitational Faraday rotation of gravitational waves by a Kerr black hole
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Black hole science with the Laser Interferometer Space Antenna
• Millisecond Magnetars
• Magnetized accretion disks around Kerr black holes with scalar hair - I. Constant angular momentum disks
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• A flexible Gaussian process reconstruction method and the mass function of the coalescing binary black hole systems
• Constraining the Initial Primordial Black Hole Clustering with CMB-distortion
• Bekenstein-Hod Universal Bound on Information Emission Rate Is Obeyed by LIGO-Virgo Binary Black Hole Remnants
• Search for Gamma-Ray Bursts and Gravitational Wave Electromagnetic Counterparts with High Energy X-ray Telescope of \textit{Insight}-HXMT
• The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
• The equation of state and some key parameters of neutron stars: constraints from GW170817, the nuclear data and the low mass X-ray binary data
• Modeling gravitational waves from exotic compact objects
• Identification of Binary Neutron Star Mergers in Gravitational-Wave Data Using YOLO One-Shot Object Detection
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• Gravitational wave constraints on spatial covariant gravities
• Hybrid stars are compatible with recent astrophysical observations
• A parametrized quasi-normal mode framework for non-Schwarzschild metrics
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Rapidly rotating neutron stars in $f(R,T)$ gravity
• Lensing of gravitational waves: universal signatures in the beating pattern
• Inspiraling double compact object detection and lensing rate -- forecast for DECIGO and B-DECIGO
• Einstein Quartic Gravity: Shadows, Signals, and Stability
• Quadratic Quasi-Normal Modes of a Schwarzschild Black Hole
• The Advanced Virgo Photon Calibrators
• Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
• Modified Gravity and the Black Hole Mass Gap
• Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1
• A note on the gravitational wave energy spectrum of parabolic and hyperbolic encounters
• Massive black holes at high redshifts from superconducting cosmic strings
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• Physics-inspired deep learning to characterize the signal manifold of quasi-circular, spinning, non-precessing binary black hole mergers
• Hadron matter in neutron stars in view of gravitational wave observations
• Detectability of modulated X-rays from LISA's supermassive black hole mergers
• Analyses of Laser Propagation Noises for TianQin Gravitational Wave Observatory Based on the Global Magnetosphere MHD Simulations
• Implications of Symmetry and Pressure in Friedmann Cosmology. II. Stellar Remnant Black Hole Mass Function
• Electromagnetic Signatures from the Tidal Tail of a Black Hole - Neutron Star Merger
• Imprint of black hole area quantization and Hawking radiation on inspiraling binary
• Mapping the Likelihood of GW190521 with Diverse Mass and Spin Priors
• Identification of Lensed Gravitational Waves with Deep Learning
• Study of eccentric binaries in Horndeski theory
• Black hole-neutron star coalescence: effects of the neutron star spin on jet launching and dynamical ejecta mass
• A GPU-accelerated mixed-precision WENO method for extremal black hole and gravitational wave physics computations
• Population-informed priors in gravitational-wave astronomy
• The new discontinuous Galerkin methods based numerical relativity program Nmesh
• BinarySkyHough: a new method to search for continuous gravitational waves from unknown neutron stars in binary systems
• Primordial black holes from cusp collapse on cosmic strings
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Constraints on primordial black holes from observation of stars in dwarf galaxies
• Neutron stars in massive scalar-Gauss-Bonnet gravity: Spherical structure and time-independent perturbations
• Primordial black holes and inflation from double-well potentials
• PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• Revisiting time delay interferometry for unequal-arm LISA and TAIJI
• Binary vision: The merging black hole binary mass distribution via iterative density estimation
• Improvement of the target sensitivity in DECIGO by optimizing its parameters for quantum noise including the effect of diffraction loss
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• Long-Term Simulations of Dynamical Ejecta: Homologous Expansion and Kilonova Properties
• Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data
• Merger rates in primordial black hole clusters without initial binaries
• Searches for Ultra-High-Energy Photons at the Pierre Auger Observatory
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Nonlinear Evolution of Quadratic Gravity in 3+1 Dimensions
• 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
• Gravitational-wave captures by intermediate-mass black holes in galactic nuclei
• Periodic orbits and gravitational wave radiation in short hair black hole spacetimes for an extreme mass ratio system
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Three approaches for the classification of protoneutron star oscillation modes
• Boson stars in Palatini $f(\mathcal{R})$ gravity
• Quantum black hole spectroscopy: probing the quantum nature of the black hole area using LIGO-Virgo ringdown detections
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• Have hierarchical three-body mergers been detected by LIGO/Virgo?
• Gravitational waves from magnetically-induced thermal neutron star mountains
• Detecting the stochastic gravitational wave background with the TianQin detector
• Bayesian parameter-estimation of Galactic binaries in LISA data with Gaussian Process Regression
• Are stellar--mass binary black hole mergers isotropically distributed?
• Searching for General Binary Inspirals with Gravitational Waves
• Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
• Merger rate of charged black holes from the two-body dynamical capture
• Gravitational wave detection without boot straps: a Bayesian approach
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the spin orientation
• Deep Generative Models of Gravitational Waveforms via Conditional Autoencoder
• Evolution of black hole shadows from superradiance
• Rapidly rotating compact stars in Rastall's gravity
• The effect of outflows on CMB bounds from Primordial Black Hole accretion
• Cosmography with Standard Sirens from the Einstein Telescope
• Primordial black holes from Higgs inflation with a Gauss-Bonnet coupling
• Exciting modes due to the aberration of gravitational waves: Measurability for extreme-mass-ratio inspirals
• A semi-supervised Machine Learning search for never-seen Gravitational-Wave sources
• Detectability of lensed gravitational waves in matched-filtering searches
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Orbital eccentricity in a neutron star - black hole merger
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Cosmic archaeology with massive stellar black hole binaries
• Detecting gravitational lensing in hierarchical triples in galactic nuclei with space-borne gravitational-wave observatories
• Lightning-Fast Gravitational Wave Parameter Inference through Neural Amortization
• Fast Parameter Estimation of Binary Mergers for Multimessenger Followup
• Threshold of Primordial Black Hole Formation against Velocity Dispersion in Matter-Dominated Era
• Impact of initial mass functions on the dynamical channel of gravitational wave sources
• Comparing Short Gamma-Ray Burst Jet Structure Models
• Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• Lepton Flavour Asymmetries and the Mass Spectrum of Primordial Black Holes
• Orbital effects on time delay interferometry for TianQin
• Detectablity of Black Hole Binaries with Gaia: Dependence on Binary Evolution Models
• Divergence in mass ratio distributions between low-mass and high-mass coalescing binary black holes
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Utilizing the null stream of the Einstein Telescope
• The anti-aligned spin of GW191109: glitch mitigation and its implications
• Forecasted constraints on modified gravity from Sunyaev Zel'dovich tomography
• Gravitational Radiation from hyperbolic encounters in the presence of dark matter
• Neutron Star Mergers as the Main Source of R-process: Natal Kicks And Inside-Out Evolution to The Rescue
• Quasinormal mode frequencies and gravitational perturbations of spinning black holes in modified gravity through METRICS: The dynamical Chern-Simons gravity case
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Time-dependent stellar-mass binary black hole mergers in AGN disks: Mass distribution of hierarchical mergers
• Gravitational wave echoes from interacting quark stars
• The Virgo O3 run and the impact of the environment
• Black hole-neutron star mergers from triples II: the role of metallicity and spin-orbit misalignment
• Moving black holes: energy extraction, absorption cross-section and the ring of fire
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
• Evidence of non-luminous matter in the center of M62
• Cryogenic suspension design for a kilometer-scale gravitational-wave detector
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
• Galactic wormholes: Geometry, stability, and echoes
• PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
• Gravitational wave source populations: Disentangling an AGN component
• Unsupervised Learning Architecture for Classifying the Transient Noise of Interferometric Gravitational-wave Detectors
• Binary neutron star formation and the origin of GW170817
• Constraining gravitational wave amplitude birefringence with GWTC-3
• The First-Order Velocity Memory Effect from Compact Binary Coalescing Sources
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Core Collapse Supernova Explosions in Active Galactic Nucleus Accretion Disks
• Tidal response and near-horizon boundary conditions for spinning exotic compact objects
• Evolution of diffuse scalar clouds around binary black holes
• Testing GR with the Gravitational Wave Inspiral Signal GW170817
• Convolutional Neural Networks for the classification of glitches in gravitational-wave data streams
• Parameter constraints on a black hole with Minkowski core through quasiperiodic oscillations
• A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing Runs
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Novel neutron decay mode inside neutron stars
• Binary Dynamics from Worldline QFT for Scalar-QED
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Of Harbingers and Higher Modes: Improved gravitational-wave early-warning of compact binary mergers
• Tidal Dissipation Impact on the Eccentric Onset of Common Envelope Phases in Massive Binary Star Systems
• LISA sources from young massive and open stellar clusters
• Prospects for Taiji to detect a gravitational-wave background from cosmic strings
• Cosmology of Supercooled Universe
• General-Relativistic Hydrodynamics Simulation of a Neutron Star - Sub-Solar-Mass Black Hole Merger
• Radio Emission from Accreting Isolated Black Holes in Our Galaxy
• Introduction to Numerical Relativity
• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Tests For Maximum Force and Maximum Power
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
• Multipole moments of compact objects with NUT charge: Theoretical and observational implications
• Fake massive black holes in the milli-Hertz gravitational-wave band
• The reliability of the low-latency estimation of binary neutron star chirp mass
• Precession and Lense-Thirring effect of hairy Kerr spacetimes
• Accurate calculation of gravitational wave memory
• Axial gravitational quasinormal modes of a self-dual black hole in loop quantum gravity
• Detecting electric charge with Extreme Mass Ratio Inspirals
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• Gravitational wave memory of the binary black hole events in GWTC-2
• Gravitational Waveform and Polarization from Binary Black Hole Inspiral in Dynamical Chern-Simons Gravity: From Generation to Propagation
• Orbital eccentricity in general relativity from catastrophe theory
• Quasi-Normal Modes of Loop Quantum Black Holes Formed from Gravitational Collapse
• 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
• Hints of spin-orbit resonances in the binary black hole population
• How important is secular evolution for black hole and neutron star mergers in 2+2 and 3+1 quadruple-star systems?
• Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• Constraining Screened Modified Gravity by Space-borne Gravitational-wave Detectors
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Multi-oscillating Boson Stars
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Constraining the Extra Polarization Modes of Gravitational Waves with Double White Dwarfs
• Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events
• Model systematics in time domain tests of binary black hole evolution
• An Isotropy Measurement with Gravitational Wave Observations
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Searching for spin-2 ULDM with gravitational waves interferometers
• Counting on Short Gamma-Ray Bursts: Gravitational-Wave Constraints of Jet Geometry
• Testing the nature of dark compact objects with gravitational waves
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Biases in estimates of black hole kicks from the spin distribution of binary black holes
• Detecting Strong Gravitational Lensing of Gravitational Waves with TianQin
• New self-force method via elliptic partial differential equations for Kerr inspiral models
• Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
• Use of Excess Power Method and Convolutional Neural Network in All-Sky Search for Continuous Gravitational Waves
• Probing the large scale structure using gravitational-wave observations of binary black holes
• The impact of distant fly-bys on the rate of binary primordial black hole mergers
• Adding higher-order spherical harmonics in non-spinning eccentric binary black hole merger waveform models
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Swift-XRT Follow-up of Gravitational Wave Triggers in the Second Advanced LIGO/Virgo Observing Run
• Neutrino flavor oscillations in stochastic gravitational waves
• Black Hole Mergers Induced by Tidal Encounters with a Galactic Centre Black Hole
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• On the Binary-Neutron-Star Post-Merger Magnetar Origin of XRT 210423
• An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Understanding binary neutron star collisions with hypermodels
• Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
• Discrepancy in tidal deformability of GW170817 between the Advanced LIGO twin detectors
• Spectral stability of near-extremal spacetimes
• Stealth black holes in shift symmetric kinetic gravity braiding
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• No static regular black holes in Einstein-complex-scalar-Gauss-Bonnet gravity
• Search for continuous gravitational waves from Fomalhaut b in the second Advanced LIGO observing run with a hidden Markov model
• Extreme mass ratio inspirals in rotating dark matter spikes
• Detecting Gravitational Self Lensing from Stellar-Mass Binaries Composed of Black Holes or Neutron Stars
• Improving the Robustness of the Advanced LIGO Detectors to Earthquakes
• Binary black hole mergers from young massive and open clusters: comparison to GWTC-2 gravitational wave data
• Fundamental physics using the temporal gravitational wave background
• Targeted search for the kinematic dipole of the gravitational-wave background
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors
• Testing black hole equatorial reflection symmetry using Sgr A* shadow images
• Endpoint of the up-down instability in precessing binary black holes
• Gravitational waveforms and radiation powers of the triple system PSR J0337+1715 in modified theories of gravity
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Electromagnetic emission from axionic boson star collisions
• Analytic Waveforms for Eccentric Gravitational Wave Bursts
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Constraints on ultra-slow-roll inflation from the third LIGO-Virgo observing run
• Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
• Calibration Uncertainty's Impact on Gravitational-Wave Observations
• Prospects for probing ultralight primordial black holes using the stochastic gravitational-wave background induced by primordial curvature perturbations
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Probing horizon scale quantum effects with Love
• Spicing up the recipe for echoes from exotic compact objects: orbital differences and corrections in rotating backgrounds
• Impact of eccentricity and mean anomaly in numerical relativity mergers
• Disc Novae: Thermodynamics of Gas Assisted Binary Black Hole Formation in AGN Discs
• Predicting the properties of black holes merger remnants with Deep Neural Networks
• A tale of tails through generalized unitarity
• Bayesian Characterisation of Circumbinary Exoplanets with LISA
• Common Envelope Wind Tunnel: Range of Applicability and Self-Similarity in Realistic Stellar Envelopes
• Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
• Search for Black Hole Merger Families
• Highly eccentric EMRI waveforms via fast self-forced inspirals
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• Interacting Kilonovae: Long-lasting Electromagnetic Counterparts to Binary Mergers in the Accretion Disks of Active Galactic Nuclei
• Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory
• Proca theory of four-dimensional regularized Gauss-Bonnet gravity and black holes with primary hair
• Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy
• Spinning Particle Dynamics and ISCO in Covariant Loop Quantum Gravity
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves
• New search pipeline for gravitational waves with higher-order modes using mode-by-mode filtering
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• Gravitational atoms in the braneworld scenario
• Hybrid Strangeon Stars
• Gravitational-Wave Searches for Cosmic String Cusps in Einstein Telescope Data using Deep Learning
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud
• 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
• The Axial Gravitational Ringing of a Spherically Symmetric Black Hole Surrounded by Dark Matter Spike
• Gravitational wave microlensing by dressed primordial black holes
• Glitch subtraction from gravitational wave data using adaptive spline fitting
• Stable vortex structures in colliding self-gravitating Bose-Einstein condensates
• Relaxing CMB bounds on Primordial Black Holes: the role of ionization fronts
• Mass$\unicode{x2013}$spin Re-Parameterization for Rapid Parameter Estimation of Inspiral Gravitational-Wave Signals
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Elliptica: a new pseudo-spectral code for the construction of initial data
• Gravitational Multipole Renormalization
• Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions
• A taxonomy of black-hole binary spin precession and nutation
• LIGO as a probe of Dark Sectors
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Universal properties of the near-horizon geometry
• Recurrent Neutrino Emission from Supermassive Black Hole Mergers
• Pandora's box lid: geometry near the apparent horizon
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• Where to find Electromagnetic Wave Counterparts of stellar-mass binary black hole mergers?
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
• Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors
• Post-merger chirps from binary black holes as probes of the final black-hole horizon
• Binary black hole growth by gas accretion in stellar clusters
• Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations
• Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Novel exact ultra-compact and ultra-sparse hairy black holes emanating from regular and phantom scalar fields
• Spin Doctors: How to diagnose a hierarchical merger origin
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Signs of Higher Multipoles and Orbital Precession in GW151226
• A scalable elliptic solver with task-based parallelism for the SpECTRE numerical relativity code
• Spontaneous creation of circularly polarized photons in chiral astrophysical systems
• Comment on "Maximum force and cosmic censorship"
• Dynamics of spinning particles in Reissner-Nordström black hole exterior
• Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
• Nucleosynthesis in outflows of compact objects and detection prospects of associated kilonovae
• The Masses of Isolated Neutron Stars Inferred from the Gravitational Redshift Measurements
• "Stairway to Heaven" -- Spectroscopy of Particle Couplings with Gravitational Waves
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• Space-borne atom interferometric gravitational wave detections. Part III. Eccentricity on dark sirens
• Constraining primordial black holes as a fraction of dark matter through accretion disk luminosity
• Lensing rates of gravitational wave signals displaying beat patterns detectable by DECIGO and B-DECIGO
• $\mu$-distortion around stupendously large primordial black holes
• Using supervised learning algorithms as a follow-up method in the search of gravitational waves from core-collapse supernovae
• Active platform stabilisation with a 6D seismometer
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• Mapping the Galactic centre's dark cluster via Resonant Relaxation
• Optimization of quantum noise by completing the square of multiple interferometer outputs in quantum locking for gravitational wave detectors
• Compact Binary Merger Rate in Dark-Matter Spikes
• Astrometric Gravitational-Wave Detection via Stellar Interferometry
• Third order post-Newtonian gravitational radiation from two-body scattering: Instantaneous energy and angular momentum radiation
• Rotating Love: The dynamical tides of spinning Newtonian stars
• Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
• Bondi-Hoyle-Lyttleton accretion onto a rotating black hole with ultralight scalar hair
• The branching ratio of LIGO binary black holes
• Prospects of joint detections of neutron star mergers and short-GRBs with Gaussian structured jets
• Implications of recoil kicks for black hole mergers from LIGO/Virgo catalogs
• Towards a real-time fully-coherent all-sky search for gravitational waves from compact binary coalescences using particle swarm optimization
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Tidal Deformability of Neutron Stars in Scalar-Tensor Theories of Gravity
• Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• Signal Space in the Triangular Network of Einstein Telescope
• Revisiting the Affleck-Dine mechanism for primordial black hole formation
• Primordial black holes: constraints, potential evidence and prospects
• Stellar Mass and Star Formation Rate within a Billion Light-Years
• Physical Implications of the Sub-threshold GRB GBM-190816 and its Associated Sub-threshold Gravitational Wave Event
• Black Hole Perturbations and Quasinormal Modes in Hybrid Metric-Palatini Gravity
• Black Hole Greybody Factors from Korteweg-de Vries Integrals: Theory
• Dark Matter Signals on a Laser Interferometer
• Gravitational wave constraints on non-birefringent dispersions of gravitational waves due to Lorentz violations with GWTC-3
• Accuracy of source localization for eccentric inspiraling binary mergers using a ground-based detector network
• Fixing the dynamical evolution of self-interacting vector fields
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass
• Multi-messenger Gravitational Lensing
• Innermost stable circular orbits in Majumdar--Papapetrou dihole spacetime
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Search for Dormant Black Holes in Ellipsoidal Variables III. The OGLE BULGE Short-Period Sample
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Inferring Parameters of GW170502: The Loudest Intermediate-mass Black Hole Trigger in LIGO's O1/O2 data
• The three body first post-Newtonian effects on the secular dynamics of a compact binary near a spinning supermassive black hole
• The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope
• Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Gravitational radiation from thermal mountains on accreting neutron stars: sources of temperature non-axisymmetry
• General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag
• The Probability Distribution of Astrophysical Gravitational-Wave Background Fluctuations
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Probing Ultralight Bosons with Compact Eccentric Binaries
• Evaluating residual acceleration noise for TianQin gravitational waves observatory with an empirical magnetic field model
• The astrophysical odds of GW151216
• H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• Influence of the Vacuum Polarization Effect on the Motion of Charged Particles in the Magnetic Field around a Schwarzschild Black Hole
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• How Do Spherical Black Holes Grow Monopole Hair?
• The H.E.S.S. Gravitational Wave Rapid Follow-up Program
• Calibrating the binary black hole population in nuclear star clusters through tidal disruption events
• Toward robust detections of nanohertz gravitational waves
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Search for gravitational waves emitted from SN 2023ixf
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Constraints on charged black holes from merger-ringdown signals in GWTC-3 and prospects for the Einstein Telescope
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• Hierarchical approach to matched filtering using a reduced basis
• Searches for Mass-Asymmetric Compact Binary Coalescence Events using Neural Networks in the LIGO/Virgo Third Observation Period
• Piezo-deformable Mirrors for Active Mode Matching in Advanced LIGO
• SN 1961V: A Pulsational Pair-Instability Supernova
• Radial and Non-Radial Oscillations of Inverted Hybrid Stars
• Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars
• Rescaling strange-cluster stars and its implications on gravitational-wave echoes
• Newtonian calibrator tests during the Virgo O3 data taking
• Silicon emissivity as a function of temperature
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• Improved inspiral-merger-ringdown model for BBHs on elliptical orbits
• Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
• Constraining properties of neutron star merger outflows with radio observations
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• Targeted modeling of GW150914's binary black hole source with dart_board
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Pulse redshift of pulsar timing array signals for all possible gravitational wave polarizations in modified general relativity
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• Up-down instability of binary black holes in numerical relativity
• Secular dynamics of binaries in stellar clusters -- III. Doubly-averaged dynamics in the presence of general relativistic precession
• Deep Learning-based Search for Microlensing Signature from Binary Black Hole Events in GWTC-1 and -2
• Linear vs. nonlinear modeling of black hole ringdowns
• Dark Stars and Gravitational Waves: Topical Review
• Magnetized accretion disks around Kerr black holes with scalar hair -- Nonconstant angular momentum disks
• 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 Comprehensive Analysis of the Gravitational Wave Events with the Hilbert-Huang Transform: From Compact Binary Coalescence to Supernova
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• SiGMa-Net: Deep learning network to distinguish binary black hole signals from short-duration noise transients
• Next-to-leading order spin-orbit effects in the equations of motion, energy loss and phase evolution of binaries of compact bodies in the effective field theory approach
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
• 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
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Bayesian model selection for GRB 211211A through multi-wavelength analyses
• Slowly Decaying Ringdown of a Rapidly Spinning Black Hole: Probing the No-Hair Theorem by Small Mass-Ratio Mergers with LISA
• Scalar induced gravitational waves in metric teleparallel gravity with the Nieh-Yan term
• Gravitational Waves in Chern-Simons-Gauss-Bonnet Gravity
• Full analytic expression of overlap reduction function for gravitational wave background with pulsar timing arrays
• Probing resonant excitations in exotic compact objects via gravitational waves
• How Do Axisymmetric Black Holes Grow Monopole and Dipole Hair?
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Exploring field-evolution and dynamical-capture coalescing binary black holes in GWTC-3
• Numerical Inside View of Hypermassive Remnant Models for GW170817
• Gravitational waves from neutron-star mountains
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Multipole tidal effects in the post-Newtonian gravitational-wave phase of compact binary coalescences
• One to many: comparing single gravitational-wave events to astrophysical populations
• Detecting dark matter oscillations with gravitational waveforms
• Homoclinic orbits in Kerr-Newman black holes
• Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves
• Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Probing Noncommutative Gravity with Gravitational Wave and Binary Pulsar Observations
• SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• Measuring Spin of the Remnant Black Hole from Maximum Amplitude
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Observational limits on the rate of radiation-driven binary black hole capture events
• The Origin of Binary Black Holes Mergers
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Repeated mergers of black hole binaries: implications for GW190521
• Black holes, stationary clouds and magnetic fields
• Premerger detection of massive black hole binaries using deep learning
• Heavy-tailed likelihoods for robustness against data outliers: Applications to the analysis of gravitational wave data
• Parameter Estimation of Gravitational Waves with a Quantum Metropolis Algorithm
• Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• GECKO Optical Follow-up Observation of Three Binary Black Hole Merger Events: GW190408_181802, GW190412, and GW190503_185404
• Influence of dark matter equation of state on the axial gravitational ringing of supermassive black holes
• Searching for gravitational waves via Doppler tracking by future missions to Uranus and Neptune
• The Irrelevance of Primordial Black Hole Clustering in the LVK mass range
• Method for environmental noise estimation via injection tests for ground-based gravitational wave detectors
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
• Intermediate mass black holes' effect on compact object binaries
• Binary Neutron Star Mergers with Missing Electromagnetic Counterparts as Manifestations of Mirror World
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• The implications of stochastic gas torques for asymmetric binaries in the LISA band
• Long-duration transient, gravitational-wave search pipeline
• New methods to assess and improve LIGO detector duty cycle
• Throat effects on strong gravitational lensing in Kerr-like wormholes
• Black hole quasinormal modes and isospectrality in Deser-Woodard nonlocal gravity
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Search for Advanced LIGO Single Interferometer Compact Binary Coalescence Signals in Coincidence with Gamma-Ray Events in Fermi-GBM
• Inconsistent black hole kick estimates from gravitational-wave models
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• Choked accretion onto a Kerr black hole
• High energy particle collisions in static, spherically symmetric black-hole-like wormholes
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Quantum back action cancellation in the audio band
• Quasinormal modes of slowly-spinning horizonless compact objects
• Gwadaptive_scattering: an automated pipeline for scattered light noise characterization
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• Did Goryachev et al. detect megahertz gravitational waves?
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves
• No slip gravity in light of LISA standard sirens
• Compact Binaries through a Lens: Silent vs. Detectable Microlensing for the LIGO-Virgo-KAGRA Gravitational Wave Observatories
• Black hole minimum size and scalar charge in shift-symmetric theories
• Modeling Compact Binary Merger Waveforms Beyond General Relativity
• Black Hole Greybody Factors from Korteweg-de Vries Integrals: Computation
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Dynamical spontaneous scalarization in Einstein-Maxwell-scalar models in anti-de Sitter spacetime
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Efficient fully precessing gravitational waveforms for binaries with neutron stars
• Gravitational wave peak luminosity model for precessing binary black holes
• ArchEnemy: Removing scattered-light glitches from gravitational wave data
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Probing modified gravitational-wave propagation through tidal measurements of binary neutron star mergers
• Enhancing interferometer sensitivity without sacrificing bandwidth and stability: beyond single-mode and resolved-sideband approximation
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Memory Effect or Cosmic String? Classifying Gravitational-Wave Bursts with Bayesian Inference
• Dynamical Instability of Self-Gravitating Membranes
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Black hole perturbations in higher-order scalar-tensor theories: initial value problem and dynamical stability
• Boosting the sensitivity of high frequency gravitational wave detectors by PT-symmetry
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Revealing the ${\chi }_{\mathrm{eff}}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Localization of gravitational waves using machine learning
• Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
• Quasinormal Modes in Modified Gravity using Physics-Informed Neural Networks
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae I: Parameter Study of the Dependence on Jet Energetics
• Population properties of neutron stars in the coalescing compact binaries
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Evidence for a strong 19.5 Hz flux oscillation in Swift BAT and Fermi GBM gamma-ray data from GRB 211211A
• Premature Black Hole Death of Population III Stars by Dark Matter
• Effect of inhomogeneities on the propagation of gravitational waves from binaries of compact objects
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• Strong clustering of primordial black holes from Affleck-Dine mechanism
• Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
• Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
• Posterior samples of the parameters of binary black holes from Advanced LIGO, Virgo's second observing run
• Gravitational wave echoes search with combs
• Implications of GWTC-3 on primordial black holes from vacuum bubbles
• Electromagnetic Emission post Spinning Black Hole-Magnetized Neutron Star Mergers
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Multi-messenger astronomy with INTEGRAL
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• An Efficient Signal to Noise Approximation for Eccentric Inspiraling Binaries
• Rapid localization of gravitational wave hosts with FIGARO
• Non-radial oscillations and gravitational wave emission of hybrid neutron stars
• New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
• Discovery of a Universal Correlation For Long and Short GRBs and Its Application on the Study of Luminosity Function and Formation Rate
• Constraining the lensing of binary neutron stars from their stochastic background
• Gravitational Waves as a Probe of the Extra Dimension
• Swarm-intelligent search for gravitational waves from eccentric binary mergers
• Dynamics of Binary System around Supermassive Black Hole
• Two-dimensional correlation function of binary black hole coalescences
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Probing supermassive black hole seed scenarios with gravitational wave measurements
• Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants
• Validating continuous gravitational-wave candidates from a semicoherent search using Doppler modulation and an effective point spread function
• Gamma-ray Diagnostics of r-process Nucleosynthesis in the Remnants of Galactic Binary Neutron-Star Mergers
• Source of black bounces in Rastall gravity
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• Matched filtering for gravitational wave detection without template bank driven by deep learning template prediction model bank
• Third post-Newtonian gravitational radiation from two-body scattering II. Hereditary Energy radiation
• On quasinormal modes in 4D black hole solutions in the model with anisotropic fluid
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Constraining black-hole binary spin precession and nutation with sequential prior conditioning
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Detection of Gravitational Waves using Parametric Resonance in Bose-Einstein Condensates
• Testing General Relativity with Gravitational Waves
• Astrophysical signal consistency test adapted for gravitational-wave transient searches
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Post-Newtonian-accurate pulsar timing array signals induced by inspiralling eccentric binaries: accuracy, computational cost, and single-pulsar search
• On the delay times of merging double neutron stars
• Deviation of geodesics and particle trajectories in a gravitational wave of the Bianchi type VI universe
• Source localizations with the network of space-based gravitational wave detectors
• Tidal effects in gravitational waves from neutron stars in scalar-tensor theories of gravity
• Motion of localized sources in general relativity: gravitational self-force from quasilocal conservation laws
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations
• The effect of Primordial Black Holes and streaming motions on structure formation
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Horndeski fermion-boson stars
• Detecting isolated stellar-mass black holes in the absence of microlensing parallax effect
• Neutrino emission upper limits with maximum likelihood estimators for joint astrophysical neutrino searches with large sky localizations
• NuSTAR observations of the unidentified INTEGRAL sources: constraints on the Galactic population of HMXBs
• Gravitational Waves from Newborn Accreting Millisecond Magnetars
• Eclipses of continuous gravitational waves as a probe of stellar structure
• r-Process enrichment in the Galactic halo characterized by nucleosynthesis variation in the ejecta of coalescing neutron star binaries
• Gravitational wave modes in matter
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• SCoRe: A New Framework to Study Unmodeled Physics from Gravitational Wave Data
• Quantum precision limits of displacement noise free interferometers
• Gravitational waves and electromagnetic radiation from charged black hole binaries
• Iterative time-domain method for resolving multiple gravitational wave sources in Pulsar Timing Array data
• Hybrid stars may have an inverted structure
• Study on the detectability of gravitational radiation from single-binary encounters between black holes in nuclear star cluster: the case of hyperbolic flybys
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Testing alternative theories of gravity with space-based gravitational wave detectors
• Constrains of the axion-like particle from black hole spin superradiance
• A phase-sensitive optomechanical amplifier for quantum noise reduction in laser interferometers
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• WIMPs in Dilatonic Einstein Gauss-Bonnet Cosmology
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Nondegenerate internal squeezing: an all-optical, loss-resistant quantum technique for gravitational-wave detection
• Beyond general relativity: designing a template-based search for exotic gravitational wave signals
• Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
• Gravitational wave cosmology I: high frequency approximation
• Searching for gravitational-wave bursts with space-borne detectors
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• The SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
• Density-clustering of continuous gravitational wave candidates from large surveys
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Revisiting Primordial Black Hole Capture by Neutron Stars
• Constraining ultra slow roll inflation using cosmological datasets
• Axial perturbations of hairy black holes in generalised scalar-tensor theories
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Analytical proof of the isospectrality of quasinormal modes for Schwarzschild-de Sitter and Schwarzschild-Anti de Sitter spacetimes
• Mind the step: On the frequency-domain analysis of gravitational-wave memory waveforms
• Electromagnetic transients and gravitational waves from white dwarf disruptions by stellar black holes in triple systems
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• A Coincidence Null Test for Poisson-Distributed Events
• Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
• A two-carrier scheme: evading the 3dB quantum penalty of heterodyne readout in gravitational-wave detectors
• Dark photon bursts from compact binary systems and constraints
• Observable Signatures of RN Black Holes with Dark Matter Halos via Strong Gravitational Lensing and Constraints from EHT Observations
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• Strong-gravity precession resonances for binary systems orbiting a Schwarzschild black hole
• Real modes and null memory contributions in effective-one-body models
• Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
• Efficient simulations of high-spin black holes with a new gauge
• Black hole spectroscopy for KAGRA future prospect in O5
• The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe
• Quantum Squeezing Schemes for Heterodyne Readout
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field model in 3+1 dimensions
• Self-interacting scalar field distributions around Schwarzschild black holes
• Search for multi-messenger signals in NOvA coincident with LIGO/Virgo detections
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Peaking into the abyss: Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• GW170817 event rules out general relativity in favor of vector gravity
• Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Searching for wormholes with gravitational wave scattering
• Hunting gravitational wave black holes with microlensing
• Primordial Black Holes without fine-tuning from a light stochastic spectator field
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• How to search for multiple messengers -- a general framework beyond two messengers
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• Impact of overlapping signals on parameterized post-Newtonian coefficients in tests of gravity
• Dictionary learning: a novel approach to detecting binary black holes in the presence of Galactic noise with LISA
• Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework
• Inferring the Astrophysical Population of Gravitational Wave Sources in the Presence of Noise Transients
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Definitions of (super) angular momentum in asymptotically flat spacetimes: Properties and applications to compact-binary mergers
• Stellar mass Primordial Black Holes as Cold Dark Matter
• Model-independent discovery prospects for primordial black holes at LIGO
• Charged black hole and radiating solutions in entangled relativity
• Abundance of LIGO/Virgo Black Holes from Microlensing Observations of Quasars with Reverberation Mapping Size Estimates
• Detection of gravitational wave mixed polarization with single space-based detectors
• Outliers in the LIGO Black Hole Mass Function from Coagulation in Dense Clusters
• Method for detecting highly-eccentric binaries with a gravitational wave burst search
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Testing the robustness of simulation-based gravitational-wave population inference
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Gravitational influence of high power laser pulses
• Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• An interference-based method for the detection of strongly lensed gravitational waves
• A Sensitive Test of Non-Gaussianity in Gravitational-wave Detector Data
• Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Effect of a second compact object on stable circular orbits
• Efficient Stochastic Template Bank using Inner Product Inequalities
• Distinguishing a stochastic gravitational-wave signal from correlated noise with joint parameter estimation: Fisher analysis for ground-based detectors
• Flavor ratios of astrophysical neutrinos interacting with stochastic gravitational waves having arbitrary spectra
• Template bank to search for exotic gravitational wave signals from astrophysical compact binaries
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• On the energetics of a possible relativistic jet associated with the binary neutron star merger candidate S190425z
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Quasinormal modes of hairy black holes in shift-symmetric theories
• Test of Kerr-Sen metric with black hole observations
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Test the Weak Cosmic Supervision Conjecture in Dark Matter-Black Hole System
• Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
• A fixed point for black hole distributions
• Action-angle variables of a binary black hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order
• Direct approach to realising quantum filters for high-precision measurements
• Electromagnetic counterparts to gravitational wave events from Gaia
• Ringdowns for black holes with scalar hair: the large mass case
• Mass and tidal parameter extraction from gravitational waves of binary neutron stars mergers using deep learning
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• A Unified $p_{\mathrm{astro}}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines
• Associating fast radio bursts with compact binary mergers via gravitational lensing
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
• Measurements of Optical Scatter Versus Annealing Temperature for Amorphous Ta2O5 and TiO2:Ta2O5 Thin Films
• Synthetic radio images of structured GRB and kilonova afterglows
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Conditional Noise Deep Learning for Parameter Estimation of Gravitational Wave Events
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
• Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement
• Characteristic formulation of the Regge-Wheeler and Zerilli Green functions
• Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
• Extending superposed harmonic initial data to higher spin
• Distortion of Gravitational-wave Signals by Astrophysical Environments
• Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• Measuring the Black Hole Mass Spectrum from Redshifts of aLIGO Binary Merger Events
• Scalar induced gravitational waves in chiral scalar-tensor theory of gravity
• New Kind of Echo from Quantum Black Holes
• Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
• Polarization modes of gravitational waves in general Einstein-vector theory
• Multidimensional hierarchical tests of general relativity with gravitational waves
• Hybrid waveforms for generic precessing binaries for gravitational-wave data analysis
• Sensors and Actuators for the Advanced LIGO+ Upgrade
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Scattering of massless bosonic fields by Kerr black holes: On-axis incidence
• ESA Voyage 2050 white paper -- Faint objects in motion: the new frontier of high precision astrometry
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• False positives for gravitational lensing: the gravitational-wave perspective
• Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
• Fundamental Physics and Cosmology with TianQin
• Systematic biases from ignoring environmental tidal effects in gravitational wave observations
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Constraining string cosmology with the gravitational-wave background using the NANOGrav 15-year data set
• Vibration Analysis of KAGRA Cryostat at Cryogenic Temperature
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Inverse problem of analog gravity systems
• Neutron Stars in the Effective Fly-By Framework: $f$-Mode Re-summation
• Black hole mass function and its evolution -- the first prediction for the Einstein Telescope
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field toy model
• Quantum limits for stationary force sensing
• Event Rate of Strongly Lensed Gravitational Waves of Stellar Binary Black Hole Mergers Produced by Dynamical Interactions
• Galaxy-Targeting Approach Optimized for Finding the Radio Afterglows of Gravitational Wave Sources
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Kicks in charged black hole binaries
• On the absence of conformally flat slicings of the Kerr spacetime
• Employing Deep Learning for Detection of Gravitational Waves from Compact Binary Coalescences
• The Sound of Clearing the Throat: Gravitational Waves from a Black Hole Orbiting in a Wormhole Geometry
• Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Initial Data and Eccentricity Reduction Toolkit for Binary Black Hole Numerical Relativity Waveforms
• Breaking black-hole uniqueness at supermassive scales
• Deep Learning for estimating parameters of Gravitational Waves
• Hyperons and $\Delta$'s in rotating protoneutron stars: Global properties
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Implementation of a generalized precession parameter in the RIFT parameter estimation algorithm
• Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• A regular metric does not ensure the regularity of spacetime
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Crustal failure as a tool to probe hybrid stars
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
• Octupolar test of general relativity
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• Probing dark matter halo profiles with multi-band observations of gravitational waves
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• Stealth black hole perturbations in kinetic gravity braiding
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• Control of a filter cavity with coherent control sidebands
• Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail
• Constraints on Brans-Dicke gravity from neutron star-black hole merger events using higher harmonics
• Improved early-warning estimates of luminosity distance and orbital inclination of compact binary mergers using higher modes of gravitational radiation
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Primordial Black-Hole-Based Pathways to Little Red Dots
• Searching for gravitational waves from stellar-mass binary black holes early inspiral
• Binary dynamics to second post-Newtonian order in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity from effective field theory
• Constraining neutron star radii in black hole-neutron star mergers from their electromagnetic counterparts
• Limiting the Abundance of LIGO/Virgo Black Holes with Microlensing Observations of Quasars of Finite Size
• Primordial black-hole formation and heavy r-process element synthesis from the cosmological QCD transition. Two aspects of an inhomogeneous early Universe
• Aberration of gravitational waveforms by peculiar velocity
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Strong and weak lensing of Gravitational Waves: a semi-analytical approach
• Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms
• The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range
• Selection rules for the decay of a particle into two identical massless particles of any spin
• Bounds on the charge of the graviton using gravitational wave observations
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Fast Radio Bursts signal high-frequency gravitational waves
• Deep-Learning Classification and Parameter Inference of Rotational Core-Collapse Supernovae
• New approach to template banks of gravitational waves with higher harmonics: Reducing matched-filtering cost by over an order of magnitude
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
• Black holes and nilmanifolds: quasinormal modes as the fingerprints of extra dimensions?
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites
• Simulating Kilonovae in the ΛCDM Universe
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Strong Equivalence Principle and Gravitational Wave Polarizations in Horndeski Theory
• Wavelet-based tools to analyze, filter, and reconstruct transient gravitational-wave signals
• Gravitational multipole moments for asymptotically de Sitter spacetimes
• Cosmology and the Early Universe
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• Adapted gauge to a quasilocal measure of the black holes recoil
• Astro2020 Decadal Science White Paper: The state of gravitational-wave astrophysics in 2020
• LIGO Signals from the Mirror World
• Measuring Mass and Radius of the Maximum-mass Nonrotating Neutron Star
• Search for UHE Photons from Gravitational Wave Sources with the Pierre Auger Observatory
• Exploring higher order images with Fe K_α-lines from relativistic disks: black hole spin determination and bias
• Unexpected LIGO events and the Mirror World
• Semianalytical Approach for Sky Localization of Gravitational Waves
• cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
• Parameterized quasinormal frequencies and Hawking radiation for axial gravitational perturbations of a holonomy-corrected black hole
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Efficient search method of anomalous reflection by the central object in an EMRI system by future space gravitational wave detectors
• Minimally-modeled search of higher multipole gravitational-wave radiation in compact binary coalescence
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• No Glitch in the Matrix: Robust Reconstruction of Gravitational Wave Signals Under Noise Artifacts
• Possibility of Primordial black holes Collision with Earth and the Consequences
• Black holes and wormholes in $f(R)$ gravity with a kinetic curvature scalar
• Gravitational Waves from Mirror World
• Exact model of gravitational wave and pure radiation
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Interaction between linear polarized plane gravitational waves and a plane electromagnetic wave in the electromagnetic-gravity analogue
• Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
• Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
• Average nonlinear dynamics of particles in gravitational pulses: effective Hamiltonian, secular acceleration, and gravitational susceptibility
• On the mass-function of GWTC-2 binary black hole systems and their progenitors
• Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• A Fisher matrix for gravitational-wave population inference
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• On the mass distribution of the LIGO-Virgo-KAGRA events
• Strong-field gravitational lensing by black holes
• Astrophysics with the Laser Interferometer Space Antenna
• Quantifying closeness between black hole spacetimes: a superspace approach
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• Black holes in torsion bigravity
• Minimally modified gravity with auxiliary constraints formalism
• Impact of signal clusters in wide-band searches for continuous gravitational waves
• Scalarization of the Reissner-Nordström black hole with higher derivative gauge field corrections
• The Timing System of LIGO Discoveries
• Are binary black hole mergers and long gamma-ray bursts drawn from the same black hole population?
• Axisymmetric Hydrodynamics in Numerical Relativity Using a Multipatch Method
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Observable-based reformulation of time-delay interferometry
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Multiple variability time-scales of the early nitrogen-rich Wolf-Rayet star WR7
• Corrections to the gravitational wave phasing
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
• Exposing Gravitational Waves below the Quantum Shot Noise
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Clockwise evolution in the hardness-intensity diagram of the black hole X-ray binary Swift J1910.2-0546
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Detectability of radio afterglows from binary neutron star mergers and implications for fast radio bursts
• Rotating black holes in valid vector-tensor theories after GW170817
• The Luminosity Distribution of Short Gamma-Ray Bursts under a Structured Jet Scenario
• Particle swarming of sensor correction filters
• Can we constrain the aftermath of binary neutron star mergers with short gamma-ray bursts?
• Life on Miller's Planet: The Habitable Zone Around Supermassive Black Holes
• TOROS Optical follow-up of the Advanced LIGO-VIRGO O2 second observational campaign
• Astro2020 Science White Paper: Radio Counterparts of Compact Object Mergers in the Era of Gravitational-Wave Astronomy
• Neutron displacement noise-free interferometer for gravitational-wave detection
• Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories
• High Frame-Rate Phase Camera for High-Resolution Wavefront Sensing in Gravitational-Wave Detectors
• Light rings in static and extremal black holes
• Prospects for the Observation of Primordial Black Hole evaporation with the Southern Wide Field of View Gamma-ray Observatory
• Novel Deep Learning Approach to Detecting Binary Black Hole Mergers
• Recent LIGO-Virgo discoveries
• Gas cooling of test masses for future gravitational-wave observatories
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
• Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources
• Can Primordial Black Holes form in the Standard Model ?
• Unbiased estimation of gravitational-wave anisotropies from noisy data
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Locally-homogeneous Riemann-Cartan geometries with the largest symmetry group
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• Building a bridge between comparable and extreme mass ratio black hole binaries: a single spin precessing model for the final state
• Probing the large-scale structure of the universe through gravitational-wave observations
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Gravitational waves in models with multicritical-point principle
• Linear stability of vector Horndeski black holes
• Demonstration of a dual-pass differential Fabry-Perot interferometer for future interferometric space gravitational wave antennas
• Well-balanced high order finite difference WENO schemes for a first-order Z4 formulation of the Einstein field equations
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• Forecast Analysis of Astrophysical Stochastic Gravitational Wave Background beyond general relativity: A Case Study on Brans-Dicke Gravity
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors
• Will Gravitational Waves Discover the First Extra-Galactic Planetary System?
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Weighing stars from birth to death: mass determination methods across the HRD
• A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
• Black Hole Merger Rates in AGN: contribution from gas-captured binaries
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• Gravitational-wave memory effects in the Damour-Esposito-Farèse extension of Brans-Dicke theory
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Multipolar Particles in Helically Symmetric Spacetimes
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• The Distributional Stress-Energy Quadrupole
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Frequency contamination from new fundamental fields in black hole ringdowns
• Exploring the Dynamics of General Relativistic Binary-Single and Binary-Binary Encounters of Black Holes
• Shrouded black holes in Einstein-Gauss-Bonnet gravity
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Optimal Gravitational-wave Follow-up Tiling Strategies Using a Genetic Algorithm
• Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity
• Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity
• Probing Particle Physics with Gravitational Waves
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT
• Enhanced power of gravitational waves and rapid coalescence of black hole binaries through dark energy accretion
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Identifying and Mitigating Machine Learning Biases for the Gravitational Wave Detection Problem
• On the Gauge Invariance of Secondary Gravitational Waves
• Eccentric mergers of binary Proca stars
• Nonlinear noise regression in gravitational-wave detectors with convolutional neural networks
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• One of Everything: The Breakthrough Listen Exotica Catalog
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• The mass, spin and rotational energy of the remnant black holes from compact binary mergers
• Observable effect of quantized cylindrical gravitational waves
• Stability analysis of the spin evolution fix points in inspiraling compact binaries with black hole, neutron star, gravastar, or boson star components
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• Arm locking in conjunction with time-delay interferometry
• Dynamical Lensing Tomography of Black Hole Ringdown
• Scalar absorption cross section of rotating black holes with tidal charge
• Evolution and detection of vector superradiant instabilities
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• Gravitational radiation back-reaction from f-modes on neutron stars
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• The NANOGrav 15 yr data set: Posterior predictive checks for gravitational-wave detection with pulsar timing arrays
• Prospects for the Observation of Continuous Gravitational Waves from Deformed Fast-spinning White Dwarfs
• Gravitational wave background from primordial black holes in globular clusters
• Improving LIGO calibration accuracy by using time-dependent filters to compensate for temporal variations
• Toward relativistic inspirals into black holes surrounded by matter
• Limiting the Number of Extra Dimensions with Shortcuts
• Effects of Short-Distance Modifications to General Relativity in Spinning Binary Systems
• Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order
• Probing eccentric higher-order modes through an effective chirp mass model
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Towards optomechanical parametric instabilities prediction in ground-based gravitational wave detectors
• Astro 2020 Science White Paper: Joint Gravitational Wave and Electromagnetic Astronomy with LIGO and LSST in the 2020's
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• The Possible Electromagnetic Counterparts of the First High-Probability NSBH Merger LIGO/Virgo S190814bv
• Beware of the running $n_s$ when producing heavy primordial black holes
• Scattering Loss in Precision Metrology due to Mirror Roughness
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Exotic compact object behavior in black hole analogues
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Closed-form solutions of spinning, eccentric binary black holes at 1.5 post-Newtonian order
• Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections
• Numerical-relativity surrogate modeling with nearly extremal black-hole spins
• UniMAP: Model-free detection of unclassified noise transients in LIGO-Virgo data using the Temporal Outlier Factor
• The effects of Galactic model uncertainties on LISA observations of double neutron stars
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• Shadowless rapidly rotating yet not ultraspinning Kerr-AdS${}_4$ and Kerr-Newman-AdS${}_4$ black holes
• Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
• Gravitational-wave imprints of Kerr--Bertotti--Robinson black holes: frequency blue-shift and waveform dephasing
• Limits on the Electro-Magnetic Counterpart of Binary Black Hole Coalescence at Visible Wavelengths
• Identifying intermediate mass binary black hole mergers in AGN disks using LISA
• 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
• 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
• Unveiling the electrodynamic nature of spacetime collisions
• On the waveform of the scalar induced gravitational waves
• Probing Binary Lens Caustics with Gravitational Waves: A Uniform Approximation Approach
• An estimate of the gravitational-wave background from the observed cosmological distribution of quasars
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• An Archival Search for Neutron-Star Mergers in Gravitational Waves and Very-High-Energy Gamma Rays
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• Strong Field Scattering of Two Black Holes: Exploring Gauge Flexibility
• Event Rate of Fast Radio Burst from Binary Neutron-star Mergers
• Thermal behavior of a radially deformed black hole spacetime
• Black hole spectroscopy of collapsing and merging neutron stars
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• A full waveform model for arbitrarily axis-symmetric black hole mergers
• Astrophysical black holes
• Deep Multimessenger Search for Compact Binary Mergers in LIGO, Virgo, and Fermi/GBM Data from 2016-2017
• Gravitational wave backgrounds from coalescing black hole binaries at cosmic dawn: an upper bound
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory
• Analysis and simulations of binary black hole merger spins -- the question of spin-axis tossing at black hole formation
• Cryogenic optical shadow sensors for future gravitational wave detectors
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Identification of Strongly Lensed Gravitational Wave Events Using Squeeze-and-Excitation Multilayer Perceptron Data-efficient Image Transformer
• Magnetic Field Simulation and Correlated Low-Frequency Noise Subtraction for an In-Orbit Demonstrator of Magnetic Measurements
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Modulations of Gravitational Waves due to Non-static Gravitational Lenses
• Gravitational Lensing of Core Collapse Supernova Gravitational Wave Signals
• Parameter estimation of binary black holes in the endpoint of the up-down instability
• Status of the Advanced Virgo gravitational-wave detector
• Stellar rotation as a new observable to test general relativity in the Galactic Center
• Multi-messenger searches via IceCube's high-energy neutrinos and gravitational-wave detections of LIGO/Virgo
• Epicyclic Frequencies for a Generic Ultracompact Object
• A Very-High-Energy Gamma-Ray View of the Transient Sky
• Alternative approach to time-delay interferometry with optical frequency comb
• Compact sources and cosmological horizons in lower dimensional bootstrapped Newtonian gravity
• Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
• Directed search for continuous gravitational waves from the possible kilonova remnant G4.8+6.2
• Ultra High Energy Neutrino Event KM3-230213A as a Signal of Electroweak Vacuum Turbulence in Merging Black Hole Binaries
• Waveform models for the gravitational-wave memory effect: Extreme mass-ratio limit and final memory offset
• Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
• Gravitational Waves from Black Holes in Merging Ultra-Dwarf Galaxies
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
• Black Holes and Wormholes in Higher-Curvature Corrected Theories of Gravity
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• Investigation of crackling noise in the vibration isolation systems of the KAGRA gravitational wave detector
• Repeated Bursts: Gravitational Waves from Highly Eccentric Binaries
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Impact of Population III stars on the astrophysical gravitational-wave background
• Gravitational radiation from birefringent matter dynamics
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Quantum Bayesian Inference with Renormalization for Gravitational Waves
• Assessing the detectability of a Stochastic Gravitational Wave Background with LISA, using an excess of power approach
• Probing Fundamental Physics with Gravitational Waves
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
• Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook
• Prospects for estimating parameters from gravitational waves of superspinar binaries
• Global Stellar Budget for LIGO Black Holes
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Extending the short gamma-ray burst population from sub-threshold triggers in Fermi/GBM and GECAM data and its implications
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Analyzing black-hole ringdowns with orthonormal modes
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• An analytical joint prior for effective spins for inference on the spin distribution of binary black holes
• Supernovae in massive binaries and compact object mergers near supermassive black holes
• Pseudospectrum of Reissner-Nordström black holes: quasinormal mode instability and universality
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Experimental investigation of the limitations of polarisation optics for future gravitational wave detectors based on the polarisation Sagnac speedmeter
• Stellar response after stripping as a model for common-envelope outcomes
• Gravitational wave echoes induced by a point mass plunging to a black hole
• Small Spins of Primordial Black Holes from Random Geometries: Bekenstein-Hawking Entropy and Gravitational Wave Observations
• A crystal ball for kilonovae
• On the angular momentum of compact binary coalescence
• Gravitational waves in Hořava-Lifshitz anisotropic gravity
• Type I Shapovalov wave spacetimes in the Brans-Dicke scalar-tensor theory of gravity
• Constraining Electromagnetic Signals from Black Holes with Hair
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Component separation map-making for stochastic gravitational wave background
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Natural polynomials for Kerr quasi-normal modes
• Microscopic State of BHs and an Exact One Body Method for Binary Dynamics in General Relativity
• Two-body problem in curved spacetime: exploring gravitational wave transient cases
• Rotations of the polarization of a gravitational wave propagating in Universe
• Evidence for Planck Luminosity Bound in Quantum Gravity
• Hairy black holes in extended Einstein-Maxwell-scalar theories with magnetic charge and kinetic couplings
• Even-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Mergers of hairy black holes: Constraining topological couplings from entropy
• Tests of general relativity at the fourth post-Newtonian order
• Extracting overlapping gravitational-wave signals of galactic compact binaries: a mini review
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Chirp mass based glitch identification in long duration gravitational wave transients
• Inferred Hubble Parameter from Gravitational Waves in a Perturbative Bianchi I Background
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• 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
• Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event
• Gravitational dynamics in a 2+1+1 decomposed spacetime along nonorthogonal double foliations: Hamiltonian evolution and gauge fixing
• Universal time delay in static spherically symmetric spacetimes for null and timelike signals
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Population Synthesis of Gravitational Wave Sources
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Constraints on the Scale Parameter of Regular Black Hole in Asymptotically Safe Gravity from Extreme Mass Ratio Inspirals
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• Constraining the environment of compact binary mergers with self-lensing signatures
• Novel black holes with scalar hair in the Einstein-Maxwell-Scalar Theory with positive coupling
• Gravitational wave propagation in generalized hybrid metric-Palatini gravity
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Scalar-induced gravitational waves in spatially covariant gravity
• A method of enhancing the detection sensitivity of transient sources in time series with Gaussian stationary noise
• Limits on the Stochastic Gravitational Wave Background and Prospects for Single Source Detection with GRACE Follow-On
• Is GW190521 a gravitational wave echo of wormhole remnant from another universe?
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Gravitational Waves and Electromagnetic Transients
• 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
• Massive boson stars: Stability and GW emission in head-on mergers
• Detectability of Electromagnetic counterparts from Neutron Star mergers: prompt emission vs afterglow
• Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping
• Metric Assisted Stochastic Sampling (MASS) search for gravitational waves from binary black hole mergers
• Detecting milli-Hz gravitational waves with optical resonators
• Determination method of binary fractions by the integrated spectrum
• Imprints of the redshift evolution of double neutron star merger rate on the signal to noise ratio distribution
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Gravitational wave pulse and memory effects for hairy Kiselev black hole and its analogy with Bondi-Sachs formalism
• A potential third-generation gravitational-wave detector based on autocorrelative weak-value amplification
• Observation of Gravitational Waves by Invariants for Electromagnetic Waves
• Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networks
• Spin and quadrupolar effects in the secular evolution of precessing compact binaries with black hole, neutron star, gravastar, or boson star components
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Space-based Gravitational Wave Observatories
• Multi-Messenger Astrophysics Opportunities with Stellar-Mass Binary Black Hole Mergers
• A novel two-mode squeezed light based on double-pump phase-matching
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Gravitational wave propagation beyond general relativity: waveform distortions and echoes
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Searching for joint neutrino and gravitational wave emission from the environment of Active Galactic Nuclei
• Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Searches for stochastic gravitational-wave backgrounds
• Search for Continuous Gravitational Wave Signals in Pulsar Timing Residuals: A New Scalable Approach with Diffusive Nested Sampling
• Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr
• Gravitational Wave Emission by Accretion of Matter and Magnetic Deformation in Fast Rotating White Dwarfs
• Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Probing chromatic onsets of gravitational wave overtones
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
• Gravitational-wave matched filtering on a quantum computer
• Statistically-informed deep learning for gravitational wave parameter estimation
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Walking along Cosmic History: Metal-poor Massive Stars
• Parameter control for binary black hole initial data
• Generalized Perturbed Kepler Problem: Gravitational Wave Imprints from Eccentric Compact Binaries
• Relative calibration of the LIGO and Virgo detectors using astrophysical events from their third observing run
• A solution of the van Dam-Veltman-Zakharov discontinuity problem in the frame of the Poincare-covariant field gravitation theory
• Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
• Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• Spin precession of binary neutron stars with magnetic dipole moments
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• Identifying the QCD Phase Transitions via the Gravitational Wave Frequency from Supernova Explosion
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• Implications of the binary coalescence events found in O1 and O2 for the stochastic background of gravitational events
• BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• Deciphering signatures of Kerr-Sen black holes in presence of plasma from the Event Horizon Telescope data
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• A Systematic Error in the Internal Friction Measurement of Coatings for Gravitational Waves Detectors
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Rigorous analytic solution to the gravitational-wave overlapping event rates
• Statistical biases in parametrized searches for gravitational-wave polarizations
• Scalable matched-filtering pipeline for gravitational-wave searches of compact binary mergers
• Detection prospects for the GW background of Galactic (sub)solar mass primordial black holes
• Lensing by primordial black holes: constraints from gravitational wave observations
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Doppler correlation-driven vetoes for the Frequency Hough analysis in continuous gravitational-wave searches
• Pearson cross-correlation in the first four black hole binary mergers
• Low-vibration cryogenic test facility for next generation of ground-based gravitational-wave observatories
• A Mass-Shell Model of Compact Binary Coalescence
• Characterization of the seismic field at Virgo and improved estimates of Newtonian-noise suppression by recesses
• Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts
• Mergers of binary neutron star systems: a multi-messenger revolution
• Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
• Linear instability of hairy black holes in Horndeski theory
• A Gravitational non-Radiative Memory Effect
• Evidence of large recoil velocity from a black hole merger signal
• Bounding dark charges on binary black holes using gravitational waves
• An introduction to gravitational waves through electrodynamics: a quadrupole comparison
• Extremely High-Order Convergence in Simulations of Relativistic Stars
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Genetic-algorithm-optimized neural networks for gravitational wave classification
• Glitch veto based on unphysical gravitational wave binary inspiral templates
• A dynamical dark energy solution to Hubble-Lemaître tension in the light of the multimessenger era
• Constraining the quantum gravity polymer scale using LIGO data
• Emission of spacetime waves from the partial collapse of a compact object
• Banks of templates for directed and all-sky narrow-band searches of continuous gravitational waves from spinning neutron stars with several spindowns
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Asymptotic Structure with vanishing cosmological constant
• Measurement of the central Galactic black hole by extremely large mass-ratio inspirals
• Group equivariant neural posterior estimation
• The Effect of Mission Duration on LISA Science Objectives
• Farside-dominant quasinuclear rainbow in refractive $\alpha$+$\alpha$ scattering
• Artificial Broadcasts as Galactic Populations: II. Comparing Individualist and Collective Bounds on Broadcast Populations in Single Galaxies
• Gamma-ray bursts at extremely small fluence
• Tidal deformations of compact objects and gravitational wave emission
• Inferring the spin distribution of binary black holes using deep learning
• Synchrotron Radio Emission as a Proxy to Identify Long Period Massive Binaries
• Expanding the Quantum-Limited Gravitational-Wave Detection Horizon
• On the effect of scalar fields on Hawking radiation and quasinormal modes of black holes
• The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
• Black hole sensitivities in Einstein-scalar-Gauss-Bonnet gravity
• Capability for detection of GW190521-like binary black holes with TianQin
• On the ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
• Density functional approach to quark matter with confinement and color superconductivity
• Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
• Quantum Physics in Space
• The influence of spin in black hole triplets
• Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
• Hierarchical search for compact binary coalescences in the Advanced LIGO's first two observing runs
• Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
• 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
• Primordial black holes from D-parity breaking in SO(10) grand unified theory
• Non canonical polarizations of Gravitational Waves
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Random projections in gravitational-wave searches from compact binaries II: efficient reconstruction of the detection statistic
• Shaken, not stirred: Test particles in binary black hole mergers
• Induced electromagnetic radiation from a charged cloud in a plane gravitational wave
• Black-box density function estimation using recursive partitioning
• Charged spherically symmetric black holes in the Lyra geometry and a preliminary investigation on the overcharging process
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
• Pure Gauss-Bonnet NUT Black Hole Solution: II
• Quantum Enhanced Interferometer for Kilohertz Gravitational Wave Detection
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• A DESGW Search for the Electromagnetic Counterpart to the LIGO/Virgo Gravitational Wave Binary Neutron Star Merger Candidate S190510g
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Predictions on observing hot holographic quark star with gravitational waves
• A template-free approach for waveform extraction of gravitational wave events
• Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass
• Prediction of the analyzing power for $\vec{p}$+${}^6$He elastic scattering at 200 MeV from $\vec{p}$+${}^4$He elastic scattering at 200 MeV
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
• Linear perturbations of dyonic black holes in the lowest-order $U(1)$ gauge-invariant scalar-vector-tensor theories
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• superB/NRPy: Scalable, Task-Based Numerical Relativity for 3G Gravitational Wave Science
• Physics beyond the Standard Model with the DSA-2000
• Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors
• Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• Examining the Gap in the Chirp Mass Distribution of Binary Black Holes
• Model-agnostic gravitational-wave background characterization algorithm
• There and back again: Outspiraling motion in non-Kerr compact objects
• Gravitational-wave constraints on noncommutative spacetime from GW190814
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data
• Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
• Where are Gaia's small black holes?
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• Exploring quantum fields in rotating black holes
• Impact of facility timing and coordination for next-generation gravitational-wave detectors
• Detecting White Dwarf Binary Mergers with Gravitational Waves
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• 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
• Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
• Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
• Probing higher curvature gravity via ringdown with overtones
• Model-agnostic search of gravitational wave echoes in LVK data
• Black-hole ringdown with templates capturing spin precession: A reanalysis of GW190521
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Formation of massive multiple-star systems: early migration and mergers
• New design of gravitational wave detectors
• Population Properties of Binary Black Holes with Eccentricity
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Circularly polarized gravitational waves from parity-violating scalar-tensor theory
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• 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
• 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
• Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
• Demonstration of length control for a filter cavity with coherent control sidebands
• Quasinormal modes of Bonanno-Reuter black holes via the Spectral Method
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Point defects in IBS coating for very low loss mirrors
• Gravitational waves from a binary source in higher dimensional spacetime with compactified extra dimensions
• Unveiling gravitational waves from core-collapse supernovae with MUSE
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Gravitational wave distance estimation using intrinsic signal properties: dark sirens as distance indicators
• A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies
• A Novel Search Technique for Low-Frequency Periodic Gravitational Waves
• The hole picture
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• Multi-Messenger Observations of GRBs: The GW connection
• Following up GW Alerts With MAGIC: The Third LIGO/Virgo Observation Run
• Gravitational wave of the Bianchi VII universe: particle trajectories, geodesic deviation and tidal accelerations
• Characterization of merging black holes with two precessing spins
• An introduction to astrophysical observables in gravitational wave detections
• The determination capability of potential neutrinos from gravitational wave sources and contributions of extra detector at the future reactor neutrino experiment
• Attenuated gravitational radiation
• MFB: A Mid-Frequency-Band Space Gravitational Wave Observer for the 2020 Decade
• An Order Statistics Post-Mortem on LIGO-Virgo GWTC-2 Events Analysed with Nested Sampling
• Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters III: limits from stellar-mass black holes using gravitational-wave observations
• Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise
• The role of longitudinal polarizations in Horndeski and macroscopic gravity: Introducing gravitational plasmas
• Dynamical double black holes and their host cluster properties
• Ultralight bosonic dark matter in white dwarfs and potential observational consequences
• Assessment of Effective-One-Body Radiation Reactions for Generic Planar Orbits
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Topological Black Holes with curvature induced scalarization in the extended scalar-tensor theories
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• Bardeen-Kiselev black hole with cosmological constant
• Discriminating between different scenarios for the formation and evolution of massive black holes with LISA
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Gravitational wave background from mergers of large primordial black holes
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• Chiral anomalies induced by gravitational waves
• EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
• Weaving the covariant three-point vertices efficiently
• The Spin and Orientation of the Black Hole in XTE J1908$+$094
• Hawking radiation by spherically-symmetric static black holes for all spins: II -- Numerical emission rates, analytical limits and new constraints
• Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background
• Correlation of Gravitational Wave Background Noises and Statistical Loss for Angular Averaged Sensitivity Curves
• The Gravity of Classical Fields: And Its Effect on the Dynamics of Gravitational Systems
• P-stars in the gravitational wave era
• Reduction of a family of metric gravities
• Parameterized tests of general relativity with gravitational wave generation and propagation
• Mitigation of Parametric Instability
• Aspects of astrophysical particle production and beyond the Standard Model phenomenology
• Concluding Remarks at the Multifrequency Behaviour of High Energy Cosmic Sources -- XIII Workshop -- II
• PatchworkWave: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe/Multimethod Simulations at Arbitrary Order
• INO: Interplanetary Network of Optical Lattice Clocks
• Higgs Field-Induced Triboluminescence in Binary Black Hole Mergers
• A fully-automated end-to-end pipeline for massive black hole binary signal extraction from LISA data