Advanced LIGO

Abstract

The Advanced LIGO gravitational wave detectors are second generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in initial LIGO, Fabry-Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal recycling has been added in Advanced LIGO to improve the frequency response. In the most sensitive frequency region around 100 Hz, the design strain sensitivity is a factor of 10 better than initial LIGO. In addition, the low frequency end of the sensitivity band is moved from 40 Hz down to 10 Hz. All interferometer components have been replaced with improved technologies to achieve this sensitivity gain. Much better seismic isolation and test mass suspensions are responsible for the gains at lower frequencies. Higher laser power, larger test masses and improved mirror coatings lead to the improved sensitivity at mid- and high- frequencies. Data collecting runs with these new instruments are planned to begin in mid-2015.

References in corpus (33)

• LIGO: The Laser Interferometer Gravitational-Wave Observatory
• Enhancing the sensitivity of the LIGO gravitational wave detector by using squeezed states of light
• Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
• A gravitational wave observatory operating beyond the quantum shot-noise limit: Squeezed light in application
• Observing binary inspiral in gravitational radiation: One interferometer
• An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin
• Quantum noise in second generation, signal-recycled laser interferometric gravitational-wave detectors
• Titania-doped tantala/silica coatings for gravitational-wave detection
• Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3
• Gravitational waves from known pulsars: results from the initial detector era
• Seismic gravity-gradient noise in interferometric gravitational-wave detectors
• Mechanical Loss in Tantala/Silica Dielectric Mirror Coatings
• All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
• Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run
• Thermoelastic Noise and Homogeneous Thermal Noise in Finite Sized Gravitational-Wave Test Masses
• Thermo-optic noise in coated mirrors for high-precision optical measurements
• DC readout experiment in Enhanced LIGO
• Subtraction of Newtonian Noise Using Optimized Sensor Arrays
• Frequency and surface dependence of the mechanical loss in fused silica
• Estimating parameters of coalescing compact binaries with proposed advanced detector networks
• Estimating parameters of coalescing compact binaries with a detector network including LIGO Australia
• Sensors and Actuators for the Advanced LIGO Mirror Suspensions
• Environmental Influences on the LIGO Gravitational Wave Detectors during the 6th Science Run
• Quantum noise in laser-interferometer gravitational-wave detectors with a heterodyne readout scheme
• A General Approach to Optomechanical Parametric Instabilities
• Long term study of the seismic environment at LIGO
• Brownian force noise from molecular collisions and the sensitivity of advanced gravitational wave observatories
• Arm-length stabilisation for interferometric gravitational-wave detectors using frequency-doubled auxiliary lasers
• Angular control of optical cavities in a radiation pressure dominated regime: the Enhanced LIGO case
• Precise calibration of LIGO test mass actuators using photon radiation pressure
• Optimal Calibration Accuracy for Gravitational Wave Detectors
• Characterization of thermal effects in the Enhanced LIGO Input Optics
• Optimal Alignment Sensing of a Readout Mode Cleaner Cavity

Cited by in corpus (2160)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• 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
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Properties of the Binary Black Hole Merger GW150914
• Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
• Is the gravitational-wave ringdown a probe of the event horizon?
• 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
• The NANOGrav 15-year Data Set: Search for Signals from New Physics
• GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
• Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
• Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei
• Squeezed states of light and their applications in laser interferometers
• Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
• GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
• The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy
• Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
• The SXS Collaboration catalog of binary black hole simulations
• Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing Run
• The Effective Field Theorist's Approach to Gravitational Dynamics
• Measuring the neutron star equation of state using X-ray timing
• Surrogate models for precessing binary black hole simulations with unequal masses
• Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
• Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
• Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO
• Testing the no-hair theorem with GW150914
• The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
• Rapid Bayesian position reconstruction for gravitational-wave transients
• Dynamical Mass Ejection from Binary Neutron Star Mergers
• A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
• GW150914: Implications for the stochastic gravitational wave background from binary black holes
• Deep Learning for Real-time Gravitational Wave Detection and Parameter Estimation: Results with Advanced LIGO Data
• Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
• AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
• On the Maximal Strength of a First-Order Electroweak Phase Transition and its Gravitational Wave Signal
• Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
• AION: An Atom Interferometer Observatory and Network
• Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
• Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
• Dynamic temperature selection for parallel-tempering in Markov chain Monte Carlo simulations
• Search for the isotropic stochastic background using data from Advanced LIGO's second observing run
• Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
• Stochastic Gravitational Wave Backgrounds
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Gravitational wave energy budget in strongly supercooled phase transitions
• Probing Ultralight Bosons with Binary Black Holes
• New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions
• 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
• Exploring gravity with the MIGA large scale atom interferometer
• Surrogate model of hybridized numerical relativity binary black hole waveforms
• Deep Neural Networks to Enable Real-time Multimessenger Astrophysics
• Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian
• Neutron star tidal deformability and equation of state constraints
• BPASS predictions for Binary Black-Hole Mergers
• Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters
• Real-time gravitational-wave science with neural posterior estimation
• Rates of Compact Object Coalescences
• GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
• Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• r-Process Lanthanide Production and Heating Rates in Kilonovae
• Stochastic and resolvable gravitational waves from ultralight bosons
• LIGO Detector Characterization in the Second and Third Observing Runs
• Black hole superradiance of self-interacting scalar fields
• Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
• Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• The cosmic merger rate of neutron stars and black holes
• Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter
• Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100)
• Low mass binary neutron star mergers : gravitational waves and neutrino emission
• Non-parametric inference of the neutron star equation of state from gravitational wave observations
• Two populations of LIGO-Virgo black holes
• Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
• Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
• Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5M_{\odot }$ Compact Object and a Neutron Star
• Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run
• 3-OGC: Catalog of gravitational waves from compact-binary mergers
• Signatures of hypermassive neutron star lifetimes on r-process nucleosynthesis in the disk ejecta from neutron star mergers
• Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• Observing gravitational-wave transient GW150914 with minimal assumptions
• Gravitational-wave cosmology across 29 decades in frequency
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• A Gravitational Wave Detector with Cosmological Reach
• Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis
• Including higher order multipoles in gravitational-wave models for precessing binary black holes
• Determining the population properties of spinning black holes
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
• General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
• Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
• A review of gravitational waves from cosmic domain walls
• Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
• Distinguishing Boson Stars from Black Holes and Neutron Stars from Tidal Interactions in Inspiraling Binary Systems
• Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
• Frequency-Dependent Squeezing for Advanced LIGO
• Deep Transfer Learning: A new deep learning glitch classification method for advanced LIGO
• Glitch Classification and Clustering for LIGO with Deep Transfer Learning
• Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations
• Constraints on cosmic strings using data from the first Advanced LIGO observing run
• Search for light scalar dark matter with atomic gravitational wave detectors
• Enhancing Gravitational-Wave Science with Machine Learning
• Prospects for doubling the range of Advanced LIGO
• Low significance of evidence for black hole echoes in gravitational wave data
• Searching for a subpopulation of primordial black holes in LIGO/Virgo gravitational-wave data
• Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
• Energetics of two-body Hamiltonians in post-Minkowskian gravity
• Gravitational-wave parameter estimation with autoregressive neural network flows
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Primordial black hole production during first-order phase transitions
• Strong gravitational lensing of explosive transients
• Probing the pre-BBN universe with gravitational waves from cosmic strings
• The BayesWave analysis pipeline in the era of gravitational wave observations
• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• Testing the binary black hole nature of a compact binary coalescence
• Nested sampling for physical scientists
• A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
• Analysis of Ringdown Overtones in GW150914
• Experimental bounds on collapse models from gravitational wave detectors
• Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
• Precise LIGO Lensing Rate Predictions for Binary Black Holes
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run
• Searching for Gravitational Waves from Compact Binaries with Precessing Spins
• Monte-Carlo simulations of black hole mergers in AGN disks: Low ${\chi }_{\mathrm{eff}}$ mergers and predictions for LIGO
• Testing general relativity using golden black-hole binaries
• Improved reconstruction of a stochastic gravitational wave background with LISA
• Convolutional neural networks: a magic bullet for gravitational-wave detection?
• Neutron-star Radius from a Population of Binary Neutron Star Mergers
• Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
• High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube
• Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies
• GW190521 as a dynamical capture of two nonspinning black holes
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• An information-theoretic approach to the gravitational-wave burst detection problem
• Upper bounds on spontaneous wave-function collapse models using millikelvin-cooled nanocantilevers
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• Binary black holes in young star clusters: the impact of metallicity
• Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order
• Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration
• Nested Sampling with Normalising Flows for Gravitational-Wave Inference
• Brane-world extra dimensions in light of GW170817
• Measuring eccentricity in binary black hole inspirals with gravitational waves
• Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
• Updated predictions for gravitational waves produced in a strongly supercooled phase transition
• Direct constraints on ultra-light boson mass from searches for continuous gravitational waves
• Phase effects from strong gravitational lensing of gravitational waves
• Tests of General Relativity with GWTC-3
• Machine-learning non-stationary noise out of gravitational wave detectors
• Blip glitches in Advanced LIGO data
• A very luminous jet from the disruption of a star by a massive black hole
• Leading higher-derivative corrections to Kerr geometry
• Searches for Continuous-Wave Gravitational Radiation
• Exploring the Early Universe with Gaia and THEIA
• The Science Case for LIGO-India
• Boson Stars and Oscillatons: A Review
• Primordial black holes and secondary gravitational waves from k/G inflation
• Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
• GEO 600 and the GEO-HF upgrade program: successes and challenges
• A Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background
• Long-lived Remnants from Binary Neutron Star Mergers
• Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
• Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914
• Asymmetric Dark Stars and Neutron Star Stability
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Observation of Parametric Instability in Advanced LIGO
• Inferring the post-merger gravitational wave emission from binary neutron star coalescences
• ELGAR -- a European Laboratory for Gravitation and Atom-interferometric Research
• The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions
• Static two-body potential at fifth post-Newtonian order
• Constraining axion inflation with gravitational waves from preheating
• Probing the Scale of New Physics by Advanced LIGO/VIRGO
• Anatomy of single-field inflationary models for primordial black holes
• Minding the gap: GW190521 as a straddling binary
• Primordial black holes and gravitational waves from parametric amplification of curvature perturbations
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• New twists in compact binary waveform modelling: a fast time domain model for precession
• General-relativistic precession in a black-hole binary
• Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases
• Low Frequency Gravitational Wave Detection With Ground Based Atom Interferometer Arrays
• Exploring the sensitivity of gravitational wave detectors to neutron star physics
• Amorphous optical coatings of present gravitational-wave interferometers
• Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
• Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
• Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA
• Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
• Probing Fundamental Physics with Gravitational Waves: The Next Generation
• Science-Driven Tunable Design of Cosmic Explorer Detectors
• Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
• Signatures of the Quantization of Gravity at Gravitational Wave Detectors
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• Black Hole Spin Constraints on the Mass Spectrum and Number of Axion-like Fields
• Low-Latency Gravitational Wave Alerts for Multi-Messenger Astronomy During the Second Advanced LIGO and Virgo Observing Run
• Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH
• Neural Importance Sampling for Rapid and Reliable Gravitational-Wave Inference
• Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
• GLADE+: An Extended Galaxy Catalogue for Multimessenger Searches with Advanced Gravitational-wave Detectors
• Directed searches for gravitational waves from ultralight bosons
• Optical Follow-up of Gravitational-wave Events with Las Cumbres Observatory
• Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO
• First low-frequency Einstein@Home all-sky search for continuous gravitational waves in Advanced LIGO data
• Standard sirens with a running Planck mass
• Discovering intermediate-mass black hole lenses through gravitational wave lensing
• On the properties of the massive binary black hole merger GW170729
• Gravitational waves and electroweak baryogenesis in a global study of the extended scalar singlet model
• Quantum Mechanics of Gravitational Waves
• The evolution of binary neutron star post-merger remnants: a review
• Continuous gravitational waves from neutron stars: current status and prospects
• Advanced LIGO detector performance in the fourth observing run
• Derivation of local-in-time fourth post-Newtonian ADM Hamiltonian for spinless compact binaries
• Frequency-Dependent Squeezed Vacuum Source for Broadband Quantum Noise Reduction in Advanced Gravitational-Wave Detectors
• All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data
• Multi-band gravitational-wave astronomy: parameter estimation and tests of general relativity with space and ground-based detectors
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• A first search for a stochastic gravitational-wave background from ultralight bosons
• Constraining axion inflation with gravitational waves across 29 decades in frequency
• Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model
• Hearing the echoes of electroweak baryogenesis with gravitational wave detectors
• GW250114: testing Hawking's area law and the Kerr nature of black holes
• Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limit
• Black Hole Mergers From Globular Clusters Observable by LISA II: Resolved Eccentric Sources and the Gravitational Wave Background
• Thanks for the memory: measuring gravitational-wave memory in the first LIGO/Virgo gravitational-wave transient catalog
• Confusing Head-On Collisions with Precessing Intermediate-Mass Binary Black Hole Mergers
• AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state
• Numerical relativity reaching into post-Newtonian territory: a compact-object binary simulation spanning 350 gravitational-wave cycles
• Constraining the orbital eccentricity of inspiralling compact binary systems with Advanced LIGO
• Electroweak bubble wall expansion: gravitational waves and baryogenesis in Standard Model-like thermal plasma
• Inferring neutron star properties from GW170817 with universal relations
• GRANDMA Observations of Advanced LIGO's and Advanced Virgo's Third Observational Campaign
• Parameter estimation with gravitational waves
• Realtime search for compact binary mergers in Advanced LIGO and Virgo's third observing run using PyCBC Live
• Black-hole spectroscopy, the no-hair theorem and GW150914: Kerr vs. Occam
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
• Parameter estimation for binary black holes with networks of third generation gravitational-wave detectors
• All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data
• GRChombo: An adaptable numerical relativity code for fundamental physics
• Black Hole Coagulation: Modeling Hierarchical Mergers in Black Hole Populations
• Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
• Constraints on ultralight scalar bosons within black hole spin measurements from LIGO-Virgo's GWTC-2
• Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
• 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
• Entanglement-Based Quantum Information Technology
• Audio-band frequency-dependent squeezing
• Interference at the Single Photon Level Along Satellite-Ground Channels
• Hidden Markov model tracking of continuous gravitational waves from a neutron star with wandering spin
• Detecting Stellar Lensing of Gravitational Waves with Ground-Based Observatories
• Reconstructing the calibrated strain signal in the Advanced LIGO detectors
• Gravitational-wave physics with Cosmic Explorer: limits to low-frequency sensitivity
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• Review of the Advanced LIGO gravitational wave observatories leading to observing run four
• A First Targeted Search for Gravitational-Wave Bursts from Core-Collapse Supernovae in Data of First-Generation Laser Interferometer Detectors
• Classical gravitational spinning-spinless scattering at $\mathcal{O}(G^2{S}^{\infty })$
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
• Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
• Mechanical loss in state-of-the-art amorphous optical coatings
• Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• Optimal probe states for the estimation of Gaussian unitary channels
• Orbital Evolution of Binaries in Circumbinary Disks
• Terrestrial Gravity Fluctuations
• Gravitational Waves from Global Cosmic Strings and Cosmic Archaeology
• Gravitational Wave and CMB Probes of Axion Kination
• Axion Dark Matter Search with Interferometric Gravitational Wave Detectors
• Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background
• Oscillons from String Moduli
• Deep-Learning continuous gravitational waves
• Search for ultralight bosons in Cygnus X-1 with Advanced LIGO
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Evidence for a minimum ellipticity in millisecond pulsars
• Studying strong phase transitions in neutron stars with gravitational waves
• The curious case of GW200129: interplay between spin-precession inference and data-quality issues
• Frequency-Dependent Responses in 3rd Generation Gravitational-Wave Detectors
• Searching for the full symphony of black hole binary mergers
• The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
• Primordial black holes and secondary gravitational waves from inflationary model with a non-canonical kinetic term
• Constraints on Einstein-dilaton-Gauss-Bonnet gravity from Black Hole-Neutron Star Gravitational Wave Events
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Noise Reduction in Gravitational-wave Data via Deep Learning
• Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
• Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Higher order gravitational-wave modes with likelihood reweighting
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• A comparison between short GRB afterglows and AT2017gfo: shedding light on kilonovae properties
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• The Influence of Neutrinos on r-Process Nucleosynthesis in the Ejecta of Black Hole-Neutron Star Mergers
• Conformal model for gravitational waves and dark matter: A status update
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• Bilby-MCMC: An MCMC sampler for gravitational-wave inference
• Intermediate mass black holes from stellar mergers in young star clusters
• Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• Searching for a Ringdown Overtone in GW150914
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism
• Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
• PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
• The effect of matter structure on the gravitational waveform
• Hearing without seeing: gravitational waves from hot and cold hidden sectors
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Search for strongly lensed counterpart images of binary black hole mergers in the first two LIGO observing runs
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Fast and Accurate Sensitivity Estimation for Continuous-Gravitational-Wave Searches
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• Hierarchical test of general relativity with gravitational waves
• A detailed analysis of GW190521 with phenomenological waveform models
• Formation channels of single and binary stellar-mass black holes
• Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers
• Black-hole ringdown as a probe of higher-curvature gravity theories
• 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
• Impact of PREX-II and combined Radio/NICER/XMM-Newton's mass-radius measurement of PSRJ0740+6620 on the dense matter equation of state
• Gravitational-wave cutoff frequencies of tidally disruptive neutron star-black hole binary mergers
• Gravitational waves from the minimal gauged $U(1{)}_{B-L}$ model
• The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• Frequency-domain gravitational waveform models for inspiraling binary neutron stars
• The first six months of the Advanced LIGO's and Advanced Virgo's third observing run with GRANDMA
• Full Band All-sky Search for Periodic Gravitational Waves in the O1 LIGO Data
• Doubly peaked induced stochastic gravitational wave background : Testing baryogenesis from primordial black holes
• Detection and Classification of Supernova Gravitational Waves Signals: A Deep Learning Approach
• The universal Teukolsky equations and black hole perturbations in higher-derivative gravity
• Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges
• Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• Inferring the population properties of binary neutron stars with gravitational-wave measurements of spin
• Gravitational wave forest from string axiverse
• Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
• Advanced quantum techniques for future gravitational-wave detectors
• Subtracting glitches from gravitational-wave detector data during the third observing run
• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
• Structure Formation and Exotic Compact Objects in a Dissipative Dark Sector
• Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data
• 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
• Measurement and subtraction of Schumann resonances at gravitational-wave interferometers
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Exploring Features in the Binary Black Hole Population
• Environmental Noise in Advanced LIGO Detectors
• Overcoming the SQL in gravitational wave detectors using spin systems with negative effective mass
• Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
• Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
• Constraints on primordial curvature perturbations from primordial black hole dark matter and secondary gravitational waves
• Modeling the postmerger gravitational wave signal and extracting binary properties from future binary neutron star detections
• Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes
• Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO
• All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems
• Search for light scalar Dark Matter candidate with AURIGA detector
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Time-dependence of the astrophysical stochastic gravitational wave background
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars
• Prospects for probing gravitational waves from primordial black hole binaries
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Neutron Star Mergers and How to Study Them
• Accelerating parameter inference with graphics processing units
• Importance of mirror modes in binary black hole ringdown waveform
• Empirical relations for gravitational-wave asteroseismology of binary neutron star mergers
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• Validating gravitational-wave detections: The Advanced LIGO hardware injection system
• The Scalar Singlet Extension of the Standard Model: Gravitational Waves versus Baryogenesis
• Prospects for detecting gravitational waves at 5 Hz with ground-based detectors
• Defining eccentricity for gravitational wave astronomy
• A Parameter-Free Tour of the Binary Black Hole Population
• Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run
• Detecting Dark Blobs
• Importance of transient resonances in extreme-mass-ratio inspirals
• An approach to computing spectral shifts for black holes beyond Kerr
• Low mechanical loss TiO${}_2$:GeO${}_2$ coatings for reduced thermal noise in Gravitational Wave Interferometers
• Sub-radian-accuracy gravitational waves from coalescing binary neutron stars II: Systematic study on the equation of state, binary mass, and mass ratio
• Gravitational spin-orbit coupling through third-subleading post-Newtonian order: from first-order self-force to arbitrary mass ratios
• 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
• On the growth of massive scalar hair around a Schwarzschild black hole
• Extracting the Gravitational Recoil from Black Hole Merger Signals
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational wave source GW150914
• Outflow Bubbles from Compact Binary Mergers Embedded in Active Galactic Nuclei: Cavity Formation and the Impact on Electromagnetic Counterparts
• Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors
• MLGWSC-1: The first Machine Learning Gravitational-Wave Search Mock Data Challenge
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• Gravitational-wave memory: waveforms and phenomenology
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers
• A fast and precise methodology to search for and analyse strongly lensed gravitational-wave events
• Constraining black hole mimickers with gravitational wave observations
• Constraints on Kerr-Newman black holes from merger-ringdown gravitational-wave observations
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Standard Siren Speeds: Improving velocities in gravitational-wave measurements of $H_0$
• Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
• Parameter estimation for black hole echo signals and their statistical significance
• Ultralight dark matter detection with mechanical quantum sensors
• First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Primordial Gravitational Wave Signals in Modified Cosmologies
• Polarization test of gravitational waves from compact binary coalescences
• GW190814: On the properties of the secondary component of the binary
• Systematic bias on parameterized tests of general relativity due to neglect of orbital eccentricity
• Hereditary Terms at Next-To-Leading Order in Two-Body Gravitational Dynamics
• Foreground cleaning and template-free stochastic background extraction for LISA
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Probing circular polarization in stochastic gravitational wave background with pulsar timing arrays
• Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM
• A Proposed Search for the Detection of Gravitational Waves from Eccentric Binary Black Holes
• Accuracy and precision of gravitational-wave models of inspiraling neutron star -- black hole binaries with spin: comparison with numerical relativity in the low-frequency regime
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• On the dynamical bar-mode instability in spinning bosonic stars
• Characterising Transient Noise in the LIGO Detectors
• Observability of lensing of gravitational waves from massive black hole binaries with LISA
• Optical suppression of tilt-to-length coupling in the LISA long-arm interferometer
• 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
• Gravitational wave and collider implications of electroweak baryogenesis aided by non-standard cosmology
• Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries
• LIGO Detector Characterization in the first half of the fourth Observing run
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• Spin dependence of black hole ringdown nonlinearities
• Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• Towards inference of overlapping gravitational wave signals
• Gravitational waves at aLIGO and vacuum stability with a scalar singlet extension of the Standard Model
• Virgo Detector Characterization and Data Quality: results from the O3 run
• Gravitational Wave Bursts as Harbingers of Cosmic Strings Diluted by Inflation
• Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine Learning
• Modeling compact binary signals and instrumental glitches in gravitational wave data
• Gravitational waves from Sco X-1: A comparison of search methods and prospects for detection with advanced detectors
• The Memory Remains (Undetected): Updates from the Second LIGO/Virgo Gravitational-Wave Transient Catalog
• Lensing of gravitational waves as a probe of compact dark matter
• Dark photon superradiance: Electrodynamics and multimessenger signals
• Modelling Double Neutron Stars: Radio and Gravitational Waves
• Uncertainty limits on neutron star radius measurements with gravitational waves
• Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
• Towards the Design of Gravitational-Wave Detectors for Probing Neutron-Star Physics
• Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• High rate of gravitational waves mergers from flyby perturbations of wide black-hole triples in the field
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• Transmuted Gravity Wave Signals from Primordial Black Holes
• The Advanced LIGO Input Optics
• Sensitivity improvements in the search for periodic gravitational waves using O1 LIGO data
• Bayesian statistical framework for identifying strongly lensed gravitational-wave signals
• Gravitational Waves from Fundamental Axion Dynamics
• Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
• Probing the seesaw scale with gravitational waves
• Shot noise in the astrophysical gravitational-wave background
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• Beating the standard sensitivity-bandwidth limit of cavity-enhanced interferometers with internal squeezed-light generation
• Binary Neutron Stars with Arbitrary Spins in Numerical Relativity
• Waveform accuracy and systematic uncertainties in current gravitational wave observations
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
• The final core collapse of pulsational pair instability supernovae
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Observable signature of merging stellar-mass black holes in active galactic nuclei
• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Status and perspectives of Continuous Gravitational Wave searches
• Modeling horizon absorption in spinning binary black holes using effective worldline theory
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• SuperRad: Modeling the black hole superradiance gravitational waveform
• Primordial black holes and secondary gravitational waves from the Higgs field
• Distinct signatures of spinning PBH domination and evaporation: doubly peaked gravitational waves, dark relics and CMB complementarity
• Dimensional Transmutation in Gravity and Cosmology
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Assessing the impact of transient orbital resonances
• Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae
• Results from the first all-sky search for continuous gravitational waves from small-ellipticity sources
• LIGOs Quantum Response to Squeezed States
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Using rational filters to uncover the first ringdown overtone in GW150914
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Gravitational waves from first-order phase transitions: Ultra-supercooled transitions and the fate of relativistic shocks
• Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes
• Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences
• A new spin on LIGO-Virgo binary black holes
• Reframing SU(1,1) interferometry
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• The SXS Collaboration's third catalog of binary black hole simulations
• Implications of the search for optical counterparts during the second part of the Advanced LIGO's and Advanced Virgo's third observing run: lessons learned for future follow-up observations
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• The time delay distribution and formation metallicity of LIGO-Virgo's binary black holes
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• Black hole spectroscopy by mode cleaning
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
• Unveiling the Dynamics of the Universe
• Search for nonlinear memory from subsolar mass compact binary mergers
• Primordial black holes and induced gravitational waves in $k$-inflation
• Eigenvalue repulsions in the quasinormal spectra of the Kerr-Newman black hole
• Statistical characterization of pulsar glitches and their potential impact on searches for continuous gravitational waves
• Black hole merger simulations in wave dark matter environments
• Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors
• On combining information from multiple gravitational wave sources
• Gravitational-wave astronomy with a physical calibration model
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• Comparing Post-Newtonian and Numerical-Relativity Precession Dynamics
• Deep Learning Ensemble for Real-time Gravitational Wave Detection of Spinning Binary Black Hole Mergers
• Laser Interferometers as Dark Matter Detectors
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• The impact of the crust equation of state on the analysis of GW170817
• Modelling the Ringdown from Precessing Black Hole Binaries
• Generation of squeezed vacuum state in the millihertz frequency band
• Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries
• Swift follow-up of the Gravitational Wave source GW150914
• Numerical simulations of stellar collapse in scalar-tensor theories of gravity
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Deep-Learning Continuous Gravitational Waves: Multiple detectors and realistic noise
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Leveraging waveform complexity for confident detection of gravitational waves
• Real-time gravitational-wave inference for binary neutron stars using machine learning
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Numerical-relativity simulations of long-lived remnants of binary neutron star mergers
• Testing General Relativity with Gravitational Waves: An Overview
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• LIGO--Virgo correlations between mass ratio and effective inspiral spin: testing the active galactic nuclei channel
• Point absorbers in Advanced LIGO
• The population properties of spinning black holes using Gravitational-wave Transient Catalog 3
• Impact of astrophysical binary coalescence timescales on the rate of lensed gravitational wave events
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• 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
• Classifying the unknown: discovering novel gravitational-wave detector glitches using similarity learning
• Do unequal-mass binary black hole systems have larger ${\chi }_{\text{eff}}$? Probing correlations with copulas in gravitational-wave astronomy
• Constraining the p-mode--g-mode tidal instability with GW170817
• Swift follow-up of gravitational wave triggers: results from the first aLIGO run and optimisation for the future
• Challenges testing the no-hair theorem with gravitational waves
• Application of hidden Markov model tracking to the search for long-duration transient gravitational waves from the remnant of the binary neutron star merger GW170817
• Spin flips in generic black hole binaries
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Ultralight vector dark matter search with auxiliary length channels of gravitational wave detectors
• Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays
• Accuracy of binary black hole waveform models for aligned-spin binaries
• Large anisotropies of the stochastic gravitational wave background from cosmic domain walls
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Dynamical tides in coalescing superfluid neutron star binaries with hyperon cores and their detectability with third generation gravitational-wave detectors
• Gravitational-Wave Lunar Observatory for Cosmology
• Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA
• Signatures of the quantum nature of gravity in the differential motion of two masses
• Importance nested sampling with normalising flows
• Limits of Astrophysics with Gravitational-Wave Backgrounds
• Centimeter-scale suspended photonic crystal mirrors
• Training Strategies for Deep Learning Gravitational-Wave Searches
• Modeling Equal and Unequal Mass Binary Neutron Star Mergers Using Public Codes
• Gravitational waves from first-order phase transitions: Towards model separation by bubble nucleation rate
• Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• Detecting stochastic gravitational waves with binary resonance
• Rapid Identification of Strongly Lensed Gravitational-Wave Events with Machine Learning
• Single field inflation in the light of Pulsar Timing Array Data: Quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition
• Small scale induced gravitational waves from primordial black holes, a stringent lower mass bound, and the imprints of an early matter to radiation transition
• Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
• Constraining the neutron-matter equation of state with gravitational waves
• Are Parametrized Tests of General Relativity with Gravitational Waves Robust to Unknown Higher Post-Newtonian Order Effects?
• Gravitational waves and the polarizations in Hořava gravity after GW170817
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Constraining extra dimensions using observations of black hole quasi-normal modes
• Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study
• Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
• (H)DPGMM: A Hierarchy of Dirichlet Process Gaussian Mixture Models for the inference of the black hole mass function
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• PhaseTracer: tracing cosmological phases and calculating transition properties
• Search for gravitational waves from high-mass-ratio compact-binary mergers of stellar mass and sub-solar mass black holes
• Scalar induced gravity waves from ultra slow-roll Galileon inflation
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
• A search for optical and near-infrared counterparts of the compact binary merger GW190814
• Systematic bias on the inspiral-merger-ringdown consistency test due to neglect of orbital eccentricity
• Lensing or luck? False alarm probabilities for gravitational lensing of gravitational waves
• A Rosetta Stone for eccentric gravitational waveform models
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Directed search for continuous gravitational-wave signals from the Galactic Center in the Advanced LIGO second observing run
• Robust semicoherent searches for continuous gravitational waves with noise and signal models including hours to days long transients
• Convolutional neural networks for the detection of the early inspiral of a gravitational-wave signal
• Binary black hole spectroscopy: a no-hair test of GW190814 and GW190412
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Constraining first-order phase transitions with curvature perturbations
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Measuring the Hubble constant with black sirens
• Direct Measurement of Coating Thermal Noise in Optical Resonators
• Hierarchical multi-stage MCMC follow-up of continuous gravitational wave candidates
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Dynamics of binary black holes in low-mass young star clusters
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Deep Residual Networks for Gravitational Wave Detection
• Convective Excitation of Inertial Modes in Binary Neutron Star Mergers
• Possible golden events for ringdown gravitational waves
• Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
• On the single-event-based identification of primordial black hole mergers at cosmological distances
• Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation
• Eigenvalue repulsions and quasinormal mode spectra of Kerr-Newman: an extended study
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• Frequency response of space-based interferometric gravitational-wave detectors
• Template Bank for Compact Binary Coalescence Searches in Gravitational Wave Data: A General Geometric Placement Algorithm
• The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity
• A Deep Search for Prompt Radio Emission from the Short GRB 150424A With The Murchison Widefield Array
• Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
• Suppressing parametric instabilities in LIGO using low-noise acoustic mode dampers
• What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
• Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
• Search for black hole hyperbolic encounters with gravitational wave detectors
• Model-Based Cross-Correlation Search for Gravitational Waves from Scorpius X-1
• Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
• Limits on hierarchical black hole mergers from the most negative ${\chi }_{\mathrm{eff}}$ systems
• Enhancement of primordial curvature perturbations in $R^3$-corrected Starobinsky-Higgs inflation
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Normalizing flows as an avenue to study overlapping gravitational wave signals
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics
• Measuring the spins of heavy binary black holes
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Global numerical simulations of the rise of vortex-mediated pulsar glitches in full general relativity
• Structure and morphology of low mechanical loss TiO${}_2$-doped Ta${}_2$O${}_5$
• Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
• New binary black hole mergers in the LIGO-Virgo O3b data
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Gravitational Spin-Orbit Hamiltonian at NNNLO in the post-Newtonian framework
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• Coherent Cancellation of Photothermal Noise in GaAs/Al${}_{0.92}$Ga${}_{0.08}$As Bragg Mirrors
• Towards the Fundamental Quantum Limit of Linear Measurements of Classical Signals
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• Quantum-enhanced interferometry for axion searches
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation
• Impacts of overlapping gravitational-wave signals on the parameter estimation: Toward the search for cosmological backgrounds
• Tail contributions to gravitational conservative dynamics
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Growth of accretion driven scalar hair around Kerr black holes
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Search of the Early O3 LIGO Data for Continuous Gravitational Waves from the Cassiopeia A and Vela Jr. Supernova Remnants
• Escape from supercooling with or without bubbles: gravitational wave signatures
• Audio-band Coating Thermal Noise Measurement for Advanced LIGO with a Multi-mode Optical Resonator
• Gravitational wave signals and cosmological consequences of gravitational reheating
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• Viewing angle of binary neutron star mergers
• Resonant Excitation of Quasinormal Modes of Black Holes
• Generation of very high-order high purity Gaussian modes via spatial light modulation
• Unveiling the merger structure of black hole binaries in generic planar orbits
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Ultra-low mass PBHs in the early universe can explain the PTA signal
• First search for long-duration transient gravitational waves after glitches in the Vela and Crab pulsars
• Completing the Fifth PN Precision Frontier via the EFT of Spinning Gravitating Objects
• Assessing the model waveform accuracy of gravitational waves
• Compact Michelson interferometers with subpicometer sensitivity
• Measuring binary black hole orbital-plane spin orientations
• Baryon and Lepton Number Violation from Gravitational Waves
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• Gravitational wave detection beyond the standard quantum limit using a negative-mass spin system and virtual rigidity
• Measuring the properties of active galactic nuclei disks with gravitational waves
• First all-sky search for continuous gravitational-wave signals from unknown neutron stars in binary systems using Advanced LIGO data
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• Localization of binary mergers with gravitational-wave detectors of second and third generation
• Testing primordial black hole and measuring the Hubble constant with multiband gravitational-wave observations
• GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle
• Gravitational traces of broken gauge symmetries
• Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• Early warning of coalescing neutron-star and neutron-star-black-hole binaries from nonstationary noise background using neural networks
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Friction on ALP domain walls and gravitational waves
• Inferring fundamental spacetime symmetries with gravitational-wave memory: from LISA to the Einstein Telescope
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• A wider look at the gravitational-wave transients from GWTC-1 using an unmodeled reconstruction method
• Implementing a semicoherent search for continuous gravitational waves using optimally-constructed template banks
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• N${}^3$LO Quadratic-in-Spin Interactions for Generic Compact Binaries
• 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
• Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data
• Results from an Einstein@Home search for continuous gravitational waves from Cassiopeia A, Vela Jr. and G347.3
• Gravitational wave propagation beyond geometric optics
• Archival searches for stellar-mass binary black holes in LISA
• Gravitational wave observations, distance measurement uncertainties, and cosmology
• Multi-waveform inference of gravitational waves
• All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
• Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
• Evidence for a correlation between binary black hole mass ratio and black-hole spins
• Finite tidal effects in GW170817: Observational evidence or model assumptions?
• Quantum expander for gravitational-wave observatories
• Angular emission patterns of remnant black holes
• N${}^3$LO Spin-Orbit Interaction via the EFT of Spinning Gravitating Objects
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• From One to Many: A Deep Learning Coincident Gravitational-Wave Search
• All-sky, all-frequency directional search for persistent gravitational-waves from Advanced LIGO's and Advanced Virgo's first three observing runs
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project
• Astrophysics with core-collapse supernova gravitational wave signals in the next generation of gravitational wave detectors
• Estimation of losses in a 300 m filter cavity and quantum noise reduction in the KAGRA gravitational-wave detector
• Cosmography using strongly lensed gravitational waves from binary black holes
• Sensitivity functions for space-borne gravitational wave detectors
• Systematic errors in estimation of gravitational-wave candidate significance
• Gravitational Quadratic-in-Spin Hamiltonian at NNNLO in the post-Newtonian framework
• Relativistic effective action of dynamical gravitomagnetic tides for slowly rotating neutron stars
• Phase transitions in perturbative walking dynamics
• Gravitational Wave Detection with Photometric Surveys
• Detectability of kilonovae in optical surveys: $post$-$mortem$ examination of the LVC O3 run follow-up
• Probing Extremal Gravitational-Wave Events with Coarse-Grained Likelihoods
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• The host galaxies of double compact objects across cosmic time
• Reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and GW170817
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Can the gravitational wave background feel wiggles in spacetime?
• SOAP: A generalised application of the Viterbi algorithm to searches for continuous gravitational-wave signals
• Probing the Black Hole Metric. I. Black Hole Shadows and Binary Black-Hole Inspirals
• Memory burden effect mimics reheating signatures on SGWB from ultra-low mass PBH domination
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: From Source to Canonical Moment
• Apparent Superluminality of Lensed Gravitational Waves
• Detection and parameter estimation challenges of Type-II lensed binary black hole signals
• Constraining early dark energy with gravitational waves before recombination
• Redshift factor and the first law of binary black hole mechanics in numerical simulations
• Pound-Drever-Hall Feedforward: Laser Phase Noise Suppression beyond Feedback
• Inferring the neutron star maximum mass and lower mass gap in neutron star-black hole systems with spin
• Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
• Cosmography with next-generation gravitational wave detectors
• All-sky search for long-duration gravitational wave transients with LIGO
• Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• Reconstructing gravitational wave signals from binary black hole mergers with minimal assumptions
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Ringdown frequencies in black holes formed from precessing black-hole binaries
• Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
• First search for ultralight dark matter with a space-based gravitational-wave antenna: LISA Pathfinder
• Measuring stochastic gravitational-wave energy beyond general relativity
• Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• DDOTI Observations of Gravitational-Wave Sources Discovered in O3
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• A new effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
• Compact binary coalescences: Constraints on waveforms
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Inferring the maximum and minimum mass of merging neutron stars with gravitational waves
• Systematic errors in estimation of gravitational-wave candidate significance
• Regression methods in waveform modeling: a comparative study
• Probing cosmological fields with gravitational wave oscillations
• 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
• Leptogenesis and Dark Matter Through Relativistic Bubble Walls with Observable Gravitational Waves
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Binary Neutron Stars Gravitational Wave Detection Based on Wavelet Packet Analysis And Convolutional Neural Networks
• Radiation-Pressure-Mediated Control of an Optomechanical Cavity
• Investigating the relation between gravitational wave tests of general relativity
• Comparison of binary black hole initial data sets
• Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
• Observing an intermediate mass black hole GW190521 with minimal assumptions
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Core collapse in massive scalar-tensor gravity
• Generalized Approach to Matched Filtering using Neural Networks
• Optimization of model independent gravitational wave search using machine learning
• Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
• Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Renormalizing Love: tidal effects at the third post-Newtonian order
• Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• Impact of correlated magnetic noise on the detection of stochastic gravitational waves: Estimation based on a simple analytical model
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning
• Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
• Optical and mechanical properties of ion-beam-sputtered Nb${}_2$O${}_5$ and TiO${}_2$-Nb${}_2$O${}_5$ thin films for gravitational-wave interferometers
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Signatures of Non-thermal Dark Matter with Kination and Early Matter Domination: Gravitational Waves versus Laboratory Searches
• Impact of high-scale Seesaw and Leptogenesis on inflationary tensor perturbations as detectable gravitational waves
• Transient gravitational waves from pulsar post-glitch recoveries
• Mountain formation by repeated, inhomogeneous crustal failure in a neutron star
• Resolving Galactic binaries using a network of space-borne gravitational wave detectors
• Gravitational Waves from Core-Collapse Supernovae
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• The next detectors for gravitational wave astronomy
• Gravitational Waves from an Inflation Triggered First-Order Phase Transition
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• Ringdown amplitudes of nonspinning eccentric binaries
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Spectral Cauchy-characteristic extraction of the gravitational wave news function
• Gravitational wave populations and cosmology with neural posterior estimation
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Full analytical formulas for frequency response of space-based gravitational wave detectors
• Bayesian semiparametric power spectral density estimation with applications in gravitational wave data analysis
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Bayesian reconstruction of gravitational wave bursts using chirplets
• Strange stars in $f(\mathcal{R})$ gravity Palatini formalism and gravitational wave echoes from them
• The detection of Quasinormal Mode of Pop III Binary Black Hole merger with final $M\sim 60M_{\odot }$ and $a/M\sim 0.7$ would confirm the strong gravity space-time around $\sim 2M$ which is only $\sim 1.17$ times the event horizon radius
• pygwb: Python-based library for gravitational-wave background searches
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• High sensitivity, levitated microsphere apparatus for short-distance force measurements
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations
• Neutron star-black hole mergers in next generation gravitational-wave observatories
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Fiducial displacements with improved accuracy for the global network of gravitational wave detectors
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
• Search for gravitational waves from twelve young supernova remnants with a hidden Markov model in Advanced LIGO's second observing run
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Prospects of gravitational-waves detections from common-envelope evolution with LISA
• GW190521: tracing imprints of spin-precession on the most massive black hole binary
• Inferring the population properties of binary black holes from unresolved gravitational waves
• 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
• Parametrizing gravitational-wave polarizations
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Gravity Spy: Lessons Learned and a Path Forward
• Exploration of co-sputtered Ta${}_2$O${}_5$-ZrO${}_2$ thin films for gravitational-wave detectors
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• Low-mass X-ray binaries from black-hole retaining globular clusters
• Probing elastic quark phases in hybrid stars with radius measurements
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• Phase-coherent mapping of gravitational-wave backgrounds using ground-based laser interferometers
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Mechanism of primordial black holes production and secondary gravitational waves in $\alpha$-attractor Galileon inflationary scenario
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence
• Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number Counts
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Observable signatures of stellar-mass black holes in active galactic nuclei
• Modified gravitational wave propagation with higher modes and its degeneracies with lensing
• An autoencoder neural network integrated into gravitational-wave burst searches to improve the rejection of noise transients
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Results from an extended Falcon all-sky survey for continuous gravitational waves
• Octupolar invariants for compact binaries on quasi-circular orbits
• Scalar-tensor mixed polarization search of gravitational waves
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Higher-order Hermite-Gauss modes as a robust flat beam in interferometric gravitational wave detectors
• Gravitational wave inference on a numerical-relativity simulation of a black hole merger beyond general relativity
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• Frequency response of time-delay interferometry for space-based gravitational wave antennas
• Loosely coherent search in LIGO O1 data for continuous gravitational waves from Terzan 5 and the galactic center
• Resonant Dampers for Parametric Instabilities in Gravitational Wave Detectors
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Noise characterization for resonantly-enhanced polarimetric vacuum magnetic-birefringence experiments
• Application of a hierarchical MCMC follow-up to Advanced LIGO continuous gravitational-wave candidates
• Combining Post-Circular and Padé approximations to compute Fourier domain templates for eccentric inspirals
• Charged Black Hole Mergers: Orbit Circularisation and Chirp Mass Bias
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• Is there an excess of black holes around $20M_{\odot }$? Optimising the complexity of population models with the use of reversible jump MCMC
• Inference of the neutron star equation of state from cosmological distances
• Simulating Transient Noise Bursts in LIGO with Generative Adversarial Networks
• Gravitational wave emission by the high braking index pulsar PSR J1640-4631
• Primordial black holes formation and secondary gravitational waves in nonminimal derivative coupling inflation
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Triaxially-deformed Freely-precessing Neutron Stars: Continuous electromagnetic and gravitational radiation
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• Universal features of gravitational waves emitted by superkick binary black hole systems
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
• Early Warnings of Binary Neutron Star Coalescence using the SPIIR Search
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• Bekenstein-Hod Universal Bound on Information Emission Rate Is Obeyed by LIGO-Virgo Binary Black Hole Remnants
• Model-Independent Radiative Symmetry Breaking and Gravitational Waves
• Stability of domain walls in models with asymmetric potentials
• Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves
• Gravitational Lensing of Gravitational Waves: Probability of Microlensing in Galaxy-Scale Lens Population
• Searching for scalar field dark matter with LIGO
• Near and far zone in two-body dynamics: an effective field theory perspective
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• Search for continuous gravitational waves from neutron stars in globular cluster NGC 6544
• Measuring tidal effects with the Einstein Telescope: A design study
• Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
• On the detection and precise localisation of merging black holes events through strong gravitational lensing
• Sensitivity of Space-based Gravitational-Wave Interferometers to Ultralight Bosonic Fields and Dark Matter
• Reduction of Classical Measurement Noise via Quantum-Dense Metrology
• Including mode mixing in a higher-multipole model for gravitational waveforms from nonspinning black-hole binaries
• PyFstat: a Python package for continuous gravitational-wave data analysis
• Super heavy dark matter origin of the PeV neutrino event: KM3-230213A
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Prospects for joint observations of gravitational waves and gamma rays from merging neutron star binaries
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Identification of Lensed Gravitational Waves with Deep Learning
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Empirically extending the range of validity of parameter-space metrics for all-sky searches for gravitational-wave pulsars
• Empirically estimating the distribution of the loudest candidate from a gravitational-wave search
• Substrate-transferred GaAs/AlGaAs crystalline coatings for gravitational-wave detectors: A review of the state of the art
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• Weyl double copy and massless free fields in curved spacetimes
• Measuring the properties of nearly extremal black holes with gravitational waves
• Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators
• Measuring the ringdown scalar polarization of gravitational waves in Einstein scalar Gauss-Bonnet gravity
• Polarized kilonovae from black hole-neutron star mergers
• PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
• Quantum correlation measurements in interferometric gravitational wave detectors
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Binary vision: The merging black hole binary mass distribution via iterative density estimation
• Probing string-inspired gravity with the inspiral-merger-ringdown consistency tests of gravitational waves
• Characterization of numerical relativity waveforms of eccentric binary black hole mergers
• The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• Maximizing the Probability of Detecting an Electromagnetic Counterpart of Gravitational-wave Events
• Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data
• Theory-agnostic framework for inspiral tests of general relativity with higher-harmonic gravitational waves
• Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches
• Cosmography with Standard Sirens from the Einstein Telescope
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• A Gravitational Wave Detector for Post Merger Neutron Stars: Beyond the Quantum Loss Limit of Michelson Fabry Perot Interferometer
• Bayesian parameter-estimation of Galactic binaries in LISA data with Gaussian Process Regression
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Detectability of Gravitational Waves from High-Redshift Binaries
• Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
• Gravitational wave detection without boot straps: a Bayesian approach
• Multi-wavelength observations of cosmological phase transitions using LISA and Cosmic Explorer
• Fundamental Limitations of Cavity-assisted Atom Interferometry
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Quantum black hole spectroscopy: probing the quantum nature of the black hole area using LIGO-Virgo ringdown detections
• Are stellar--mass binary black hole mergers isotropically distributed?
• A frequency resolved atlas of the sky in continuous gravitational waves
• Domain walls and gravitational waves in the Standard Model
• Orbital eccentricity in a neutron star - black hole merger
• Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
• Gravitational Radiation from hyperbolic encounters in the presence of dark matter
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Searching for High Frequency Gravitational Waves with Phonons
• The Virgo O3 run and the impact of the environment
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Search strategies for long gravitational-wave transients: hidden Markov model tracking and seedless clustering
• The anti-aligned spin of GW191109: glitch mitigation and its implications
• Detecting gravitational lensing in hierarchical triples in galactic nuclei with space-borne gravitational-wave observatories
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Fourth LIGO-Virgo-KAGRA Observing Run
• Utilizing the null stream of the Einstein Telescope
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• Observational Selection Effects with Ground-based Gravitational Wave Detectors
• Probing microplasticity in small scale FCC crystals via Dynamic Mechanical Analysis
• Tetrads in SU(N) Yang-Mills geometrodynamics
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• Gaussian Processes for Glitch-robust Gravitational-wave Astronomy
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Detectability of lensed gravitational waves in matched-filtering searches
• Gravitational waves from dark matter collapse in a star
• Magnetic-distortion-induced ellipticity and gravitational wave radiation of neutron stars: millisecond magnetars in short GRBs, Galactic pulsars, and magnetars
• Efficient resummation of high post-Newtonian contributions to the binding energy
• A basic introduction to ultrastable optical cavities for laser stabilization
• Gravitational wave source populations: Disentangling an AGN component
• Exploring gravitational-wave detection and parameter inference using Deep Learning methods
• Cryogenic suspension design for a kilometer-scale gravitational-wave detector
• Self-force correction to geodetic spin precession in Kerr spacetime
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• Multiple Hierarchies from a Warped Extra Dimension
• Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
• Unsupervised Learning Architecture for Classifying the Transient Noise of Interferometric Gravitational-wave Detectors
• Observing the Shadows of Stellar-Mass Black Holes with Binary Companions
• ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
• Constraining gravitational wave amplitude birefringence with GWTC-3
• Probing the speed of gravity with LVK, LISA, and joint observations
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• Least square ellipsoid fitting using iterative orthogonal transformations
• Search for transient gravitational waves in coincidence with short duration radio transients during 2007-2013
• Updated detection prospects for relic neutrinos using coherent scattering
• Parameter estimation of a two-component neutron star model with spin wandering
• Gravitational Wave Signatures of Lepton Universality Violation
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Technology for the next gravitational wave detectors
• Convolutional Neural Networks for the classification of glitches in gravitational-wave data streams
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals from Black-hole Perturbation Approach
• Using machine learning to parametrize postmerger signals from binary neutron stars
• Localization of Binary Black-Hole Mergers with Known Inclination
• Converting the signal-recycling cavity into an unstable optomechanical filter to enhance the detection bandwidth of gravitational-wave detectors
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Synthetic FM triplet for AM-free precision laser stabilization and spectroscopy
• Effect of orbital eccentricity on the dynamics of precessing compact binaries
• Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• Cosmic string gravitational waves from global $U(1{)}_{B-L}$ symmetry breaking as a probe of the type I seesaw scale
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• General-Relativistic Hydrodynamics Simulation of a Neutron Star - Sub-Solar-Mass Black Hole Merger
• Particle swarm optimization of the sensitivity of a cryogenic gravitational wave detector
• On the equal-mass limit of precessing black-hole binaries
• Hints of spin-orbit resonances in the binary black hole population
• Enhanced curvature perturbations from spherical domain walls nucleated during inflation
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
• High-accuracy simulations of highly spinning binary neutron star systems
• A fully-coherent all-sky search for gravitational-waves from compact binary coalescences
• GW150914: First search for the electromagnetic counterpart of a gravitational-wave event by the TOROS collaboration
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
• GWitchHunters: Machine Learning and citizen science to improve the performance of Gravitational Wave detector
• Constraining neutron star properties with a new equation of state insensitive approach
• Arm locking performance with the new LISA design
• Searching for spin-2 ULDM with gravitational waves interferometers
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Rapid parameter estimation for an all-sky continuous gravitational wave search using conditional varitational auto-encoders
• Tidal heating as a direct probe of strangeness inside neutron stars
• Pre-merger sky localization of gravitational waves from binary neutron star mergers using deep learning
• Slaying Axion-Like Particles via Gravitational Waves and Primordial Black Holes from Supercooled Phase Transition
• Upper limits on the Polarized Isotropic Stochastic Gravitational-Wave Background from Advanced LIGO-Virgo's First Three Observing Runs
• Generalised gravitational burst generation with Generative Adversarial Networks
• Frequency- and polarization-dependent lensing of gravitational waves in strong gravitational fields
• Biases in estimates of black hole kicks from the spin distribution of binary black holes
• Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Prospects for detecting transient quasi-monochromatic gravitational waves from glitching pulsars with current and future detectors
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Gravitational Wave Timing Array
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Observational prospects of self-interacting scalar superradiance with next-generation gravitational-wave detectors
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• An Isotropy Measurement with Gravitational Wave Observations
• Deep exploration for continuous gravitational waves at 171--172 Hz in LIGO second observing run data
• From the EFT of Spinning Gravitating Objects to Poincaré and Gauge Invariance at the 4.5PN Precision Frontier
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Reconstructing Gravitational Wave Core-Collapse Supernova Signals with Dynamic Time Warping
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• Rapid model comparison of equations of state from gravitational wave observation of binary neutron star coalescences
• Inferring neutron star properties with continuous gravitational waves
• On Improving the Performance of Glitch Classification for Gravitational Wave Detection by using Generative Adversarial Networks
• The Multi-mode Acoustic Gravitational Wave Experiment: MAGE
• Stochastic Gravitational Waves from Post-inflationary Structure Formation
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Identifying strongly lensed gravitational waves through their phase consistency
• Gravitational waves from small spin-up and spin-down events of neutron stars
• Probing phase transition in neutron stars via the crust-core interfacial mode
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Calibration Uncertainty's Impact on Gravitational-Wave Observations
• Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
• Search for continuous gravitational waves from Fomalhaut b in the second Advanced LIGO observing run with a hidden Markov model
• Sensitivity to Dark Sector Scales from Gravitational Wave Signatures
• Frequency planning for LISA
• Searching for Gamma-Ray counterparts to Gravitational Waves from merging binary neutron stars with the Cherenkov Telescope Array
• Virgo Detector Characterization and Data Quality: tools
• Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources
• The fate of twin stars on the unstable branch: implications for the formation of twin stars
• Establishing significance of gravitational-wave signals from a single observatory in the PyCBC offline search
• Probing neutron star structure via f-mode oscillations and damping in dynamical spacetime models
• A classifier for gravitational-wave inspiral signals in non-ideal single-detector data
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Prospects for probing ultralight primordial black holes using the stochastic gravitational-wave background induced by primordial curvature perturbations
• Fundamental physics using the temporal gravitational wave background
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
• Dipolar tidal effects in gravitational waves from scalarized black hole binary inspirals in quadratic gravity
• Radiation Reaction for Non-Spinning Bodies at 4.5PN in the Effective Field Theory Approach
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• Resampling to accelerate cross-correlation searches for continuous gravitational waves from binary systems
• GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
• Gravitational Wave Astronomy: Delivering on the Promises
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• Stability of the protoneutron stars toward black hole formation
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Ripples in Spacetime from Broken Supersymmetry
• Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors
• Probing general relativistic spin-orbit coupling with gravitational waves from hierarchical triple systems
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Gravitational-Wave Searches for Cosmic String Cusps in Einstein Telescope Data using Deep Learning
• LIGO as a probe of Dark Sectors
• A lower limit for Newtonian-noise models of the Einstein Telescope
• Performance of Particle Swarm Optimization on the fully-coherent all-sky search for gravitational waves from compact binary coalescences
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
• Sensing Optical Cavity Mismatch with a Mode-Converter and Quadrant Photodiode
• Detectability and parameter estimation of GWTC-3 events with LISA
• A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
• Optimising the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
• Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• Probing Left-Right Symmetry via Gravitational Waves from Domain Walls
• Gravitational waves from pulsars with measured braking index
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Analyzing black-hole ringdowns II: data conditioning
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Glitch subtraction from gravitational wave data using adaptive spline fitting
• Self-Interacting Gravitational Atoms in the Strong-Gravity Regime
• Gravitational Multipole Renormalization
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• Forecasts on interacting dark energy with standard sirens
• Seismic Cross-coupling Noise in Torsion Pendulums
• Using supervised learning algorithms as a follow-up method in the search of gravitational waves from core-collapse supernovae
• Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data
• Constraints on new physics around the MeV scale with cosmological observations
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• Prospects of joint detections of neutron star mergers and short-GRBs with Gaussian structured jets
• Spin Hall effects in the sky
• Ultra-deep tidal disruption events: prompt self-intersections and observables
• Detecting non-Gaussian gravitational wave backgrounds: a unified framework
• Continuous Gravitational Waves: A New Window to Look for Heavy Non-annihilating Dark Matter
• Squeezed light at 2128 nm for future gravitational-wave observatories
• The Palomar Transient Factory Sky2Night programme
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Mergers of Maximally Charged Primordial Black Holes
• Spin Doctors: How to diagnose a hierarchical merger origin
• Gravitational Wave Opacity from Gauge Field Dark Energy
• KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
• Results from an Einstein@Home search for continuous gravitational waves from G347.3 at low frequencies in LIGO O2 data
• Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
• Search for Long-duration Gravitational-wave Signals Associated with Magnetar Giant Flares
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Binary Black Hole Merger Rates Inferred from Luminosity Function of Ultra-Luminous X-ray Sources
• Dark Black Holes in the Mass Gap
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• Ternary Quarter Wavelength Coatings for Gravitational Wave Detector Mirrors: Design Optimization via Exhaustive Search
• "Stairway to Heaven" -- Spectroscopy of Particle Couplings with Gravitational Waves
• Defining eccentricity for spin-precessing binaries
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• Opportunities and limits of lunar gravitational-wave detection
• The astrophysical odds of GW151216
• Observable Gravitational Waves from Hyperkination in Palatini Gravity and Beyond
• Supermassive Binary Black Hole Evolution can be traced by a small SKA Pulsar Timing Array
• Angular Resolution of the Search for Anisotropic Stochastic Gravitational-Wave Background with Terrestrial Gravitational-Wave Detectors
• Multi-spatial-mode effects in squeezed-light-enhanced interferometric gravitational wave detectors
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Search for eccentric NSBH and BNS mergers in the third observing run of Advanced LIGO and Virgo
• Multi-messenger Gravitational Lensing
• Analytic thin wall false vacuum decay rate
• Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• The Linear Regime of Tachyonic Preheating
• Detecting Fundamental Vector Fields with LISA
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Novel directed search strategy to detect continuous gravitational waves from neutron stars in low- and high-eccentricity binary systems
• Consistent eccentricities for gravitational wave astronomy: Resolving discrepancies between astrophysical simulations and waveform models
• Signal Space in the Triangular Network of Einstein Telescope
• A stochastic search for intermittent gravitational-wave backgrounds
• Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain
• Sensitivity study using machine learning algorithms on simulated r-mode gravitational wave signals from newborn neutron stars
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Convolutional neural network search for long-duration transient gravitational waves from glitching pulsars
• The three body first post-Newtonian effects on the secular dynamics of a compact binary near a spinning supermassive black hole
• Effects of orbital precession on hyperbolic encounters
• Hierarchical Bayesian method for detecting continuous gravitational waves from an ensemble of pulsars
• Magnetic coupling to the Advanced Virgo payloads and its impact on the low frequency sensitivity
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Naturally small neutrino mass with asymptotic safety and gravitational-wave signatures
• Exploring Supernova Gravitational Waves with Machine Learning
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Dilated convolutional neural network for detecting extreme-mass-ratio inspirals
• Bayesian search for gravitational wave bursts in pulsar timing array data
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• 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
• Measurement of the Cross-Correlation Angular Power Spectrum Between the Stochastic Gravitational Wave Background and Galaxy Over-Density
• Evidence of the pair instability gap from black hole masses
• A waveform model for the missing quadrupole mode from black hole coalescence: memory effect and ringdown of the $(\ell =2,m=0)$ spherical harmonic
• Nonchaotic evolution of triangular configuration due to gravitational radiation reaction in the three-body problem
• Dynamical quasinormal mode excitation
• Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• Imprint of PBH domination on gravitational waves generated by cosmic strings
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Implications of the Quantum Noise Target for the Einstein Telescope Infrastructure Design
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• Improved inspiral-merger-ringdown model for BBHs on elliptical orbits
• Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
• Matrix Heater in the Gravitational Wave Observatory GEO 600
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• Silicon emissivity as a function of temperature
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• Bayesian modelling of scattered light in the LIGO interferometers
• Late-time tails in nonlinear evolutions of merging black holes
• Possible binary neutron star merger history of the primary of GW230529
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Piezo-deformable Mirrors for Active Mode Matching in Advanced LIGO
• SiGMa-Net: Deep learning network to distinguish binary black hole signals from short-duration noise transients
• Ultrafast quantum light uncertainty dynamics in real time
• Applying the Viterbi Algorithm to Planetary-Mass Black Hole Searches
• 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
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Targeted modeling of GW150914's binary black hole source with dart_board
• Scalarization of isolated black holes in scalar Gauss-Bonnet theory in the fixing-the-equations approach
• A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• BOSS-LDG: A Novel Computational Framework that Brings Together Blue Waters, Open Science Grid, Shifter and the LIGO Data Grid to Accelerate Gravitational Wave Discovery
• Observational Signatures of Highly Magnified Gravitational Waves from Compact Binary Coalescence
• Search for gravitational waves emitted from SN 2023ixf
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• Nonlinear gravitational-wave memory from cusps and kinks on cosmic strings
• Calibrating gravitational-wave detectors with GW170817
• Self-Gravity Effects of Ultralight Boson Clouds Formed by Black Hole Superradiance
• Characterization of low-significance gravitational-wave compact binary sources
• Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• Bistability-assisted Mechanical Squeezing and Entanglement
• Untangling PBH overproduction in $w$-SIGWs generated by Pulsar Timing Arrays for MST-EFT of single field inflation
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• Experimental demonstrations of alignment and mode matching in optical cavities with higher-order Hermite-Gauss modes
• Prompt sky localization of compact binary sources using a meshfree approximation
• Measuring Spin of the Remnant Black Hole from Maximum Amplitude
• Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• Neutron stars formation and Core Collapse Supernovae
• Heavy-tailed likelihoods for robustness against data outliers: Applications to the analysis of gravitational wave data
• One to many: comparing single gravitational-wave events to astrophysical populations
• Probing the Origin of Primordial Black Holes through Novel Gravitational Wave Spectrum
• First-order phase transitions in Twin Higgs models
• Measuring neutron-star distances and properties with gravitational-wave parallax
• Exploring the CPT violation and birefringence of gravitational waves with ground- and space-based gravitational-wave interferometers
• Detection of Low Tension Cosmic Superstrings
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Waterfall stiff period can generate observable primordial gravitational waves
• Constraining the Gravitational-Wave Spectrum from Cosmological First-Order Phase Transitions Using Data from LIGO-Virgo First Three Observing Runs
• Gravitational waves from neutron-star mountains
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Ranking Candidate Signals with Machine Learning in Low-Latency Search for Gravitational-Waves from Compact Binary Mergers
• Observational limits on the rate of radiation-driven binary black hole capture events
• HEALPix Alchemy: Fast All-Sky Geometry and Image Arithmetic in a Relational Database for Multimessenger Astronomy Brokers
• Template Lattices for a Cross-Correlation Search for Gravitational Waves from Scorpius X-1
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Towards observing the neutron star collapse with gravitational wave detectors
• Numerical Inside View of Hypermassive Remnant Models for GW170817
• Probing resonant excitations in exotic compact objects via gravitational waves
• Technologies for the ELGAR large scale atom interferometer array
• Searching for MHz Gravitational Waves from Harmonic Sources
• Prediction of crystallized phases of amorphous Ta${}_2$O${}_5$-based mixed oxide thin films using density functional theory calculations
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• The Quantum Memory Matrix: A Unified Framework for the Black Hole Information Paradox
• Precision Ephemerides for Gravitational-wave Searches -- IV: Corrected and refined ephemeris for Scorpius X-1
• Achieving the fundamental quantum limit of linear waveform estimation
• Primordial Gravitational Waves as Probe of Dark Matter in Interferometer Missions: Fisher Forecast and MCMC
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches
• Time-frequency track distance for comparing continuous gravitational wave signals
• The Impact of Black Hole Scaling Relation Assumptions on the Mass Density of Black Holes
• Inconsistent black hole kick estimates from gravitational-wave models
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
• ArchEnemy: Removing scattered-light glitches from gravitational wave data
• Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
• Gravitational wave peak luminosity model for precessing binary black holes
• Efficient fully precessing gravitational waveforms for binaries with neutron stars
• Gwadaptive_scattering: an automated pipeline for scattered light noise characterization
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Impact of combinations of time-delay interferometry channels on stochastic gravitational wave background detection
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Long-duration transient, gravitational-wave search pipeline
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• Observational implications of lowering the LIGO-Virgo alert threshold
• (P)reheating and gravitational waves in $\alpha$-attractor models
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• The Zadko Telescope: Exploring the transient Universe
• Tracking continuous gravitational waves from a neutron star at once and twice the spin frequency with a hidden Markov model
• Transition of EMRIs through resonance: corrections to higher order in the on-resonance flux modification
• The False Alarms induced by Gaussian Noise in Gravitational Wave Detectors
• Quantum Estimation of Parameters of Classical Spacetimes
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Did Goryachev et al. detect megahertz gravitational waves?
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Thermal charge carrier driven noise in transmissive semiconductor optics
• Domain walls in the extensions of the Standard Model
• Doppler effect in TianQin time-delay interferometry
• Optimal detuning for quantum filter cavities
• Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Scalaroca stars: coupled scalar-Proca solitons
• GROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline
• Neutron star mass in dark matter clumps
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• Bilinear noise subtraction at the GEO 600 observatory
• Single-element dual-interferometer for precision inertial sensing
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves
• Mitigating the binary viewing angle bias for standard sirens
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Systematic calibration error requirements for gravitational-wave detectors via the Cramér-Rao bound
• A method for the experimental measurement of bulk and shear loss angles in amorphous thin films
• An analysis and visualization of the output mode-matching requirements for squeezing in Advanced LIGO and future gravitational wave detectors
• Formation of GW230529 from Isolated Binary Evolution
• Mode matching error signals using radio-frequency beam shape modulation
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors
• Scale-invariant spin dynamics and the quantum limits of field sensing
• Quasinormal Modes in Modified Gravity using Physics-Informed Neural Networks
• Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope
• High Precision Inertial Sensors on a One Inch Diameter Optic
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Macroscopic quantum entanglement between an optomechanical cavity and a continuous field in presence of non-Markovian noise
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• Optical Gravitational Wave Antenna with Increased Power Handling Capability
• LOFAR 144-MHz follow-up observations of GW170817
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Detectability of gravitational higher order modes in the third-generation era
• Localization of gravitational waves using machine learning
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Validating continuous gravitational-wave candidates from a semicoherent search using Doppler modulation and an effective point spread function
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Templated Anisotropic Analyses of the LISA Galactic Foreground
• Stochastic gravitational wave background: birth from string-wall death
• An observational upper limit on the rate of gamma-ray bursts with neutron star-black hole merger progenitors
• Gravitational Waves from Mini-Split SUSY
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• Rapid localization of gravitational wave hosts with FIGARO
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Macroscopic Dark Matter Detection with Gravitational Wave Experiments
• Numerical convergence of model Cauchy-characteristic extraction and matching
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses
• Possible confirmation of the existence of ergoregion by the Kerr quasinormal mode in gravitational waves from Pop III massive black hole binary
• Information Retrieval and Recommendation System for Astronomical Observatories
• Astrophysical signal consistency test adapted for gravitational-wave transient searches
• Parametrized tests of general relativity using eccentric compact binaries
• The detectability of single spinless stellar-mass black holes through gravitational lensing of gravitational waves with advanced LIGO
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Statistical Measures of Planck Scale Signal Correlations in Interferometers
• Rapid gravitational wave parameter estimation with a single spin: Systematic uncertainties in parameter estimation with the SpinTaylorF2 approximation
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• Mind the step: On the frequency-domain analysis of gravitational-wave memory waveforms
• Testing the nature of GW200105 by probing the frequency evolution of eccentricity
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge
• A two-carrier scheme: evading the 3dB quantum penalty of heterodyne readout in gravitational-wave detectors
• An optimal ${\chi }^2$ discriminator against modelled noise-transients in interferometric data in searches for binary black-hole mergers
• Constrains of the axion-like particle from black hole spin superradiance
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Study on the detectability of gravitational radiation from single-binary encounters between black holes in nuclear star cluster: the case of hyperbolic flybys
• Quantum precision limits of displacement noise free interferometers
• Testing pseudo-complex general relativity with gravitational waves
• Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
• Nondegenerate internal squeezing: an all-optical, loss-resistant quantum technique for gravitational-wave detection
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Training Process of Unsupervised Learning Architecture for Gravity Spy Dataset
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• $2\cdot 10^{-13}$ fractional laser frequency stability with a 7-cm unequal-arm Mach-Zehnder interferometer
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Bubble nucleation and gravitational wave from holography
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• - Gravitational Waves - A Review on the Conceptual Foundations of Gravitational Radiation
• Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• Generalized analysis of quantum noise and dynamic back-action in signal-recycled Michelson-type laser interferometers
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Crossed optical cavities with large mode diameters
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Gravitational waves from axions annihilation through quantum field theory
• Cosmological Consequences of Domain Walls Biased by Quantum Gravity
• Method to detect gravitational waves from an ensemble of known pulsars
• A Coincidence Null Test for Poisson-Distributed Events
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Fast control of atom-light interaction in a narrow linewidth cavity
• Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order
• Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
• Towards a Precision Measurement of Binary Black Holes Formation Channels Using Gravitational Waves and Emission Lines
• Bounds on tidal charges from gravitational-wave ringdown observations
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Reduction of quantum noise using the quantum locking with an optical spring for gravitational wave detectors
• Real modes and null memory contributions in effective-one-body models
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Seismic Background Limitation of Lunar Gravitational-wave Detectors
• Negative dispersion medium at 1064 nm in an optomechanical resonator for enhancing the sensitivity bandwidth in a gravitational-wave detector
• Reexamining Evidence of a Pair-Instability Mass Gap in the Binary Black Hole Population
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak
• Optimal Sensor Fusion Method for Active Vibration Isolation Systems in Ground-Based Gravitational-Wave Detectors
• Quantum signature of gravity in optomechanical systems with conditional measurement
• What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Coherent coupling completes an unambiguous optomechanical classification framework
• Template bank to search for exotic gravitational wave signals from astrophysical compact binaries
• A neural network emulator of the Advanced LIGO and Advanced Virgo selection function
• Probing flavor violation and baryogenesis via primordial gravitational waves
• A convolutional neural network to distinguish glitches from minute-long gravitational wave transients
• Assessing the impact of non-Gaussian noise on convolutional neural networks that search for continuous gravitational waves
• Distinguishing a stochastic gravitational-wave signal from correlated noise with joint parameter estimation: Fisher analysis for ground-based detectors
• Development of ion-beam sputtered silicon nitride thin films for low-noise mirror coatings of gravitational-wave detectors
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Effects of mirror birefringence and its fluctuations to laser interferometric gravitational wave detectors
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Efficient Stochastic Template Bank using Inner Product Inequalities
• Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping
• Estimation of the gravitational wave polarizations from a non template search
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Detectability of strongly lensed gravitational waves using model-independent image parameters
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Parameter Estimation with Nonstationary Noise in Gravitational-wave Data
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
• Detection of gravitational wave mixed polarization with single space-based detectors
• Quantum Squeezing Schemes for Heterodyne Readout
• Method for detecting highly-eccentric binaries with a gravitational wave burst search
• Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
• Gravitational wave astrophysics, data analysis and multimessenger astronomy
• Accelerated detection of the binary neutron star gravitational-wave background
• Dictionary learning: a novel approach to detecting binary black holes in the presence of Galactic noise with LISA
• Obtaining Gravitational Waves from Inspiral Binary Systems using LIGO data
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• The detection of quasinormal mode with $a/M\sim 0.95$ would prove a sphere $99\%$ soaking in the ergoregion of the Kerr space-time
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Testing the robustness of simulation-based gravitational-wave population inference
• Search for continuous gravitational waves from PSR J0437$-$4715 with a hidden Markov model in O3 LIGO data
• No evidence for a dip in the binary black hole mass spectrum
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• An interference-based method for the detection of strongly lensed gravitational waves
• False positives for gravitational lensing: the gravitational-wave perspective
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Multidimensional hierarchical tests of general relativity with gravitational waves
• Universal relations to measure neutron star properties from targeted r-mode searches
• Search for Postmerger Gravitational Waves from Binary Neutron Star Mergers Using a Matched-filtering Statistic
• Lensing and wave optics in the strong field of a black hole
• Associating fast radio bursts with compact binary mergers via gravitational lensing
• Measurements of Optical Scatter Versus Annealing Temperature for Amorphous Ta2O5 and TiO2:Ta2O5 Thin Films
• Demonstration of an amplitude filter cavity at gravitational-wave frequencies
• A Unified $p_{\mathrm{astro}}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines
• Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Ultralight boson constraints from gravitational wave observations of spinning binary black holes
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Misalignment and mode mismatch error signals for higher-order Hermite-Gauss modes from two sensing schemes
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Optimizing StackSlide setup and data selection for continuous-gravitational-wave searches in realistic detector data
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Effects of Galaxy Cluster Structure on Lensed Gravitational Waves
• Dissipative coupling, dispersive coupling and their combination in the cavity-less opto-mechanical systems
• Swift X-ray Follow-Up Observations of Gravitational Wave and High-Energy Neutrino Coincident Signals
• Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
• B-modes from Post-inflationary Gravitational Waves Sourced by Axionic Instabilities at Cosmic Reionization
• Non-modal effects in black hole perturbation theory: Transient Superradiance
• Graphics processing unit implementation of the F-statistic for continuous gravitational wave searches
• Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
• Astrophysical Source Classification and Distance Estimation for PyCBC Live
• Vibration Analysis of KAGRA Cryostat at Cryogenic Temperature
• Negative non-Gaussianity as a salvager for PBHs with PTAs in bounce
• Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order
• Higher-order tails and RG flows due to scattering of gravitational radiation from binary inspirals
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Neutron Stars in the Effective Fly-By Framework: $f$-Mode Re-summation
• Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
• Thermal leptogenesis, dark matter, and gravitational waves from an extended canonical seesaw scenario
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• A model-independent tripartite test of cosmic distance relations
• Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
• Half-solution to the two-body problem in General Relativity
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
• Early warning of precessing neutron-star black-hole binary mergers with the near-future gravitational-wave detectors
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
• Quasi-periodic oscillation in short gamma-ray bursts from black hole-neutron star mergers
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• A laser interferometer accelerometer for vibration sensitive cryogenic experiments
• Path integral action for a resonant detector of gravitational waves in the generalized uncertainty principle framework
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Binary dynamics to second post-Newtonian order in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity from effective field theory
• Improving the stability of frequency dependent squeezing with bichromatic control of filter cavity length, alignment and incident beam pointing
• The Fourier Transform of the Continuous Gravitational Wave Signal
• Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA
• Bounds on the charge of the graviton using gravitational wave observations
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Search for stochastic gravitational-wave background from string cosmology with Advanced LIGO and Virgo's O1$\sim$O3 data
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Fast Frequency-Domain Effective Fly-By Waveforms
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Gravitational wave polarization from combined Earth-space detectors
• Selection Effects in Periodic X-ray Data from Maximizing Detection Statistics
• Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n-vector ensemble method
• Estimation of Newtonian noise from KAGRA cooling system
• PeV-scale leptogenesis, gravity waves and black holes from a SUSY-breaking phase transition
• Observational constraint on axion dark matter in a realistic halo profile with gravitational waves
• Improved early-warning estimates of luminosity distance and orbital inclination of compact binary mergers using higher modes of gravitational radiation
• Constraints on Brans-Dicke gravity from neutron star-black hole merger events using higher harmonics
• Modeling circulating cavity fields using the discrete linear canonical transform
• Post-Newtonian Dynamics of Spinning Black Hole Binaries in Einstein-Scalar-Gauss-Bonnet Gravity
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Unveiling the Universe with Emerging Cosmological Probes
• Gravitational Lensing in the Charged NUT-de Sitter Spacetime
• Imaging Scatterometer for Observing In-Situ Changes to Optical Coatings During Air Annealing
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Unification of thermal and quantum noise in gravitational-wave detectors
• Enhancing gravitational waveform models through dynamic calibration
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Cavity-enhanced polarization rotation measurements for low-disturbance probing of atoms
• The curvature dependence of gravitational-wave tests of General Relativity
• Beyond the Horizon Distance: LIGO-Virgo can Boost Gravitational Wave Detection Rates by Exploiting the Mass Distribution of Neutron Stars
• Convolutional Neural Networks for signal detection in real LIGO data
• Using Schroedinger cat quantum state for detection of a given phase shift
• Implementation of a generalized precession parameter in the RIFT parameter estimation algorithm
• Deep Learning for estimating parameters of Gravitational Waves
• Piecewise frequency model for searches for long-transient gravitational waves from young neutron stars
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Effects of transients in LIGO suspensions on searches for gravitational waves
• Exploring dark photons via a subfrequency laser searchin gravitational wave detectors
• Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail
• Angular correlation and deformed Hellings-Downs curve from spin-2 ultralight dark matter
• Two sides of the same coin: the F-statistic and the 5-vector method
• Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
• Impact of the cosmic neutrino background on black hole superradiance
• Compact integrated optical sensors and electromagnetic actuators for vibration isolation systems in the gravitational-wave detector KAGRA
• Precessing Binary Black Holes as Better Dark Sirens
• Non-thermal production of heavy vector dark matter from relativistic bubble walls
• Multimessenger hierarchical triple merger gravitational-wave event pair GW190514-GW190521 inside AGN J124942.3 + 344929
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• Astrophysics with the Laser Interferometer Space Antenna
• A High-Finesse Suspended Interferometric Sensor for Macroscopic Quantum Mechanics with Femtometre Sensitivity
• Linear dynamics and classical tests of the gravitational quantum field theory
• Toward the detection of gravitational waves under non-Gaussian noises II. Independent Component Analysis
• An in-situ method for measuring the non-linear response of a Fabry-Perot cavity
• Reducing controls noise in gravitational wave detectors with interferometric local damping of suspended optics
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Minimally modified gravity with auxiliary constraints formalism
• The effect of noise artefacts on gravitational-wave searches for neutron star post-merger remnants
• Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data
• Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
• Enhancing the sensitivity of interferometers with stable phase-insensitive quantum filters
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• Point Absorber Limits to Future Gravitational-Wave Detectors
• What do gravitational wave detectors say about polymer quantum effects?
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Minimally-modeled search of higher multipole gravitational-wave radiation in compact binary coalescence
• Model-independent search for anisotropies in stochastic gravitational-wave backgrounds and application to LIGO-Virgo's first three observing Runs
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• First-step experiment in developing optical-spring quantum locking for DECIGO: sensitivity optimization for simulated quantum noise by completing the square
• Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
• Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology
• Cosmic superstrings in large volume compactifications: PTAs, LISA and time-varying tension
• Geometric Approach to Analytic Marginalisation of the Likelihood Ratio for Continuous Gravitational Wave Searches
• Simulating Kilonovae in the ΛCDM Universe
• Interaction between linear polarized plane gravitational waves and a plane electromagnetic wave in the electromagnetic-gravity analogue
• The Timing System of LIGO Discoveries
• Polymer quantization and advanced gravitational wave detector
• A Common Origin for Low Mass Ratio Events Observed by LIGO and Virgo in the First Half of the Third Observing Run
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• Targeted Search for Gravitational Waves from Highly Spinning Light Compact Binaries
• Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
• Gravitational waves from cosmic strings for pedestrians
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?
• Search for continuous gravitational waves directed at sub-threshold radiometer candidates in O3 LIGO data
• Massive fields affected by echoes: New physics vs. astrophysical environment
• Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
• Probing charge of compact objects with gravitational microlensing of gravitational waves
• cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
• Numerical Relativity Multimodal Waveforms using Absorbing Boundary Conditions
• Dual balanced readout for scattered light noise mitigation in Michelson interferometers
• Angular instability in high optical power suspended cavities
• Inferring small neutron star spins with neutron star-black hole mergers
• Reconstruction of binary black hole harmonics in LIGO using deep learning
• Memory of a Random Walk: Astrometric deflections from gravitational wave memory accumulation over cosmological scales
• Dynamic motion trajectory control with nanoradian accuracy for multi-element X-ray optical systems via laser interferometry
• Observability of spin precession in the presence of a black-hole remnant kick
• GPU-accelerated Image Reduction Pipeline
• On the mass distribution of the LIGO-Virgo-KAGRA events
• High Speed Source Localization in Searches for Gravitational Waves from Compact Object Collisions
• Characterization of gravitational-wave detector noise with fractals
• Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2
• Navigating Unknowns: Deep Learning Robustness for Gravitational Wave Signal Reconstruction
• A directed continuous-wave search from Scorpius X-1 with the five-vector resampling technique
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• Passive-performance, analysis, and upgrades of a 1-ton seismic attenuation system
• Constraining temperature distribution inside LIGO test masses from frequencies of their vibrational modes
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• Recent LIGO-Virgo discoveries
• A high angular resolution interferometric backscatter meter
• Observational constraint on axion dark matter with gravitational waves
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Optical losses as a function of beam position on the mirrors in a 285-m suspended Fabry-Perot cavity
• Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass
• Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Detection of GW200105 with a targeted eccentric search
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity
• Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Diffraction around caustics in gravitational wave lensing
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• Gravitational-Wave Signatures of Nonstandard Neutrino Properties in Collapsing Stellar Cores
• A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
• A search using GEO600 for gravitational waves coincident with fast radio bursts from SGR 1935+2154
• Accelerated parameter estimation of supermassive black hole binaries in LISA using a meshfree approximation
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Integrating high-precision and fringe-scale displacement sensing using heterodyne cavity-tracking
• Crescendo Beyond the Horizon: More Gravitational Waves from Domain Walls Bounded by Inflated Cosmic Strings
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• lenscat: a Public and Community-Contributed Catalog of Known Strong Gravitational Lenses
• Primordial Black Holes and Gravitational Waves in the $U(1{)}_{B-L}$ Extended Inert Doublet Model: A First-Order Phase Transition Perspective
• Toward a computationally-efficient follow-up pipeline for blind continuous gravitational-wave searches
• New semicoherent targeted search for continuous gravitational waves from pulsars in binary systems
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Gravitational Wave Probe of Primordial Black Hole Origin via Superradiance
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Novel Deep Learning Approach to Detecting Binary Black Hole Mergers
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• Revisiting Thermal Charge Carrier Refractive Noise in Semiconductor Optics for Gravitational-Wave Interferometers
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Response of the underground environment of the KAGRA observatory against the air-pressure disturbance from the Tonga volcano eruption on January 15th, 2022
• Exposing Gravitational Waves below the Quantum Shot Noise
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Combination of dissipative and dispersive coupling in the cavity optomechanical systems
• Neutron displacement noise-free interferometer for gravitational-wave detection
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Calibration of Advanced Virgo and reconstruction of detector strain h(t) during the Observing Run O3
• Fast Radio Bursts as crustal dynamical events induced by magnetic field evolution in young magnetars
• High Frame-Rate Phase Camera for High-Resolution Wavefront Sensing in Gravitational-Wave Detectors
• Gas cooling of test masses for future gravitational-wave observatories
• Optimal Gravitational-wave Follow-up Tiling Strategies Using a Genetic Algorithm
• A Three-Dimensional Laser Interferometer Gravitational-Wave Detector
• TOROS Optical follow-up of the Advanced LIGO-VIRGO O2 second observational campaign
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Driving unmodelled gravitational-wave transient searches using astrophysical information
• Gravitational Wave Searches for Aligned-Spin Binary Neutron Stars Using Nonspinning Templates
• Primordial gravitational waves from spontaneous Lorentz symmetry breaking
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Realization of Gain with Electromagnetically Induced Transparency System with Non-degenerate Zeeman Sublevels in ${}^{87}$Rb
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Improving LIGO calibration accuracy by using time-dependent filters to compensate for temporal variations
• Optimized localization for gravitational-waves from merging binaries
• Probing Supermassive Black Hole Binaries with Orbital Resonances of Laser-Ranged Satellite
• Strong lensing of gravitational waves with modified propagation
• Numerical-relativity surrogate modeling with nearly extremal black-hole spins
• Random projections in gravitational wave searches of compact binaries
• Can a "pure vector" gravitational wave mimic a "pure tensor" one?
• Uncovering faint lensed gravitational-wave signals and reprioritizing their follow-up analysis using galaxy lensing forecasts with detected counterparts
• Neutron Stars, Ungravity, and the I-Love-Q relation
• Probing black hole `charge' from the binary black hole inspiral
• Trajectories without quantum uncertainties in composite systems with disparate energy spectra
• Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
• Review of Conformally Flat Approximation for Binary Neutron Star Initial Conditions
• Critical Quantum Sensing: a tutorial on parameter estimation near quantum phase transitions
• Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order
• Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
• Classification uncertainty for transient gravitational-wave noise artefacts with optimised conformal prediction
• Primordial black holes and magnetic fields in conformal neutrino mass models
• Towards optomechanical parametric instabilities prediction in ground-based gravitational wave detectors
• WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event
• The directional isotropy of LIGO-Virgo binaries
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Phase decomposition of the template metric for continuous gravitational-wave searches
• Spectrogram correlated stacking: A novel time-frequency domain analysis of the Stochastic Gravitational Wave Background
• Probing eccentric higher-order modes through an effective chirp mass model
• Scalar Gravitational Wave Signals from Core Collapse in Massive Scalar-Tensor Gravity with Triple-Scalar Interactions
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Machine Learning for Quantum-Enhanced Gravitational-Wave Observatories
• Observing the optical modes of parametric instability
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
• Analytic weak-signal approximation of the Bayes factor for continuous gravitational waves
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• 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
• Gravitational wave imprints on spontaneous emission
• Identifying multichannel coherent couplings and causal relationships in gravitational wave detectors
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Looking To The Horizon: Probing Evolution in the Black Hole Spectrum With Gravitational Wave Catalogs
• Profiling stellar environments of gravitational wave sources
• Colloquium: Multimessenger astronomy with continuous gravitational waves and future detectors
• Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation
• Gravitational waves from superradiant instabilities of rotating black holes
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Evolution and detection of vector superradiant instabilities
• Arm locking in conjunction with time-delay interferometry
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Strategies to reduce the thermoelastic loss of multimaterial coated finite substrates
• Constraining self-interactions of a massive scalar field using scalar gravitational waves from stellar core collapse
• Searching for Anisotropy in the Gravitational Wave Background Using the Parkes Pulsar Timing Array
• Assessing the similarity of continuous gravitational-wave signals to narrow instrumental artifacts
• Identifying and Mitigating Machine Learning Biases for the Gravitational Wave Detection Problem
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• UniMAP: Model-free detection of unclassified noise transients in LIGO-Virgo data using the Temporal Outlier Factor
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Effects of Short-Distance Modifications to General Relativity in Spinning Binary Systems
• Achieving the Multi-parameter Quantum Cramér-Rao Bound with Antiunitary Symmetry
• Numerical Relativity and the Discovery of Gravitational Waves
• Quantum sensors with matter waves for GW observation
• MALBEC: a new CUDA-C ray-tracer in General Relativity
• Probing Binary Lens Caustics with Gravitational Waves: A Uniform Approximation Approach
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• Thermal modulation for suppression of parametric instability in advanced gravitational wave detectors
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• A prototype differential atom interferometer for fundamental physics
• Joint inference for gravitational wave signals and glitches using a data-informed glitch model
• Inferring the spins of merging black holes in the presence of data-quality issues
• Conceptual design and science cases of a juggled interferometer for gravitational wave detection
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
• Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Identification of Strongly Lensed Gravitational Wave Events Using Squeeze-and-Excitation Multilayer Perceptron Data-efficient Image Transformer
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• Electroweak Phase Transition, Gravitational Waves and Collider Probes in Multi-Scalar Dark Matter Scenarios
• Chiral gravitational waves from thermalized neutrinos in the early Universe
• Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Detecting gravitational waves with light
• Suppressing data anomalies of gravitational reference sensors with time delay interferometry combinations
• A characterization method for low-frequency environmental noise in LIGO
• Measuring $H_0$ with pulsar timing arrays
• Improved binary black hole searches through better discrimination against noise transients
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Sky localization of space-based detectors with time-delay interferometry
• Prospects for estimating parameters from gravitational waves of superspinar binaries
• Development of advanced photon calibrator for Kamioka gravitational wave detector (KAGRA)
• Maximum mass and stability of differentially rotating neutrons stars
• Eccentric Catastrophes & What To Do With Them
• Extending the short gamma-ray burst population from sub-threshold triggers in Fermi/GBM and GECAM data and its implications
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Deep Multimessenger Search for Compact Binary Mergers in LIGO, Virgo, and Fermi/GBM Data from 2016-2017
• Extracting electromagnetic signatures of spacetime fluctuations
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• The prospects of gravitational waves on constraining the anisotropy of the Universe
• Efficient representations of upper limits and confidence intervals for experimental data
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Gravitational wave signals from long lasting binary-single black hole encounters
• Optimizing the low-latency localization of gravitational waves
• Binary Black Hole Information Loss Paradox & Future Prospects
• On the Astrophysical Origin of Binary Black Hole Subpopulations: A Tale of Three Channels?
• Regularization of a scalar charged particle for generic orbits in Kerr spacetime
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Multi-messenger searches via IceCube's high-energy neutrinos and gravitational-wave detections of LIGO/Virgo
• A compact actively damped vibration isolation platform for optical experiments in ultra-high vacuum
• Rates and beaming angles of GRBs associated with compact binary coalescences
• Gravitational Wave Duet by Resonating Binary Black Holes within Ultralight Dark Matter
• Gravitational waves from a curvature-induced phase transition of a Higgs-portal dark matter sector
• Generative adversarial network for stellar core-collapse gravitational waves
• Measuring the speed of gravity and the cosmic expansion with time delays between gravity and light from binary neutron stars
• Search for continuous gravitational waves from unknown neutron stars in binary systems with long orbital periods in O3 data
• Response of interferometers to the vacuum of quantum gravity
• Black-Hole Cartography
• Influence of gravitational waves upon light in the Minkowski background: from null geodesics to interferometry
• Thermal noise of beam splitters in laser gravitational wave detectors
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• An Archival Search for Neutron-Star Mergers in Gravitational Waves and Very-High-Energy Gamma Rays
• Spontaneous crystallization noise in mirrors of gravitational wave detectors
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Testing hilltop supernatural inflation with gravitational waves
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• GW231123: Overlapping Gravitational Wave Signals?
• Spin-up and mass-gain in hyperbolic encounters of spinning black holes
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Sensing and vetoing loud transient noises for the gravitational-wave detection
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• Discrete $R$-symmetry, Various Energy Scales and Gravitational Waves
• Universality of stationary entanglement in an optomechanical system driven by non-Markovian noise and squeezed light
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Optimal Design of Coatings for Mirrors of Gravitational Wave Detectors: Analytic Turbo Solution via Herpin Equivalent Layers
• Gravitational Wave Spectral Shapes as a probe of Long Lived Right-handed Neutrinos, Leptogenesis and Dark Matter: Global versus Local B-L Cosmic Strings
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Particle Conversions Beyond the WKB Approximation and Solar-Induced Gravitational Waves from Dark Photon Dark Matter
• Comparing astrophysical models to gravitational-wave data in the observable space
• RADAR-Radio Afterglow Detection and AI-driven Response: A Federated Framework for Gravitational Wave Event Follow-Up
• Using t-SNE for characterizing glitches in LIGO detectors
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Co-interacting dark matter and conformally coupled light scalars
• A weakly-modeled search for compact binary coalescences in Einstein Telescope
• Effects of dynamical capture on two equal-mass nonspinning black holes
• Systematic errors in low latency gravitational wave parameter estimation impact electromagnetic follow-up observations
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• An analytical joint prior for effective spins for inference on the spin distribution of binary black holes
• Transformer Networks for Continuous Gravitational-wave Searches
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networks
• Effects of orbital eccentricity on continuous gravitational waveforms from triaxially deformed precessing neutron stars in tight binaries
• Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Discovering gravitational waveform distortions from lensing: A deep dive into GW231123
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Computing spectral shifts for Johannsen-Psaltis black holes
• Sky localization of gravitational waves from eccentric binaries
• Fundamental quantum limits for detecting ultrahigh frequency gravitational waves
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• Machine-directed gravitational-wave counterpart discovery
• Probing the equation of state of neutron stars with captured primordial black holes
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Astrophysical Evidence of Wakefield Acceleration in Galactic and Extragalactic Jets via Gamma Rays and UHECRs
• Sensing and control scheme for the inteferometer configuration with an L-shaped resonator
• Gravitational waves from axion inflation in the gradient expansion formalism. Part II. Fermionic axion inflation
• Exploring the viability of pseudo Nambu-Goldstone boson as ultralight dark matter in a mass range relevant for strong gravity applications
• Searching for topological dark matter in LIGO data
• Looking for ancillary signals around GW150914
• Beam displacement tolerances on a segmented mirror for higher-order Hermite-Gauss modes
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• A Pseudo Plane-wave Gravitational Calibrator for Gravitational Wave Observatories
• Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers
• Glitches far from transient gravitational-wave events do not bias inference
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Do black holes remember what they are made of?
• Detecting milli-Hz gravitational waves with optical resonators
• One-stop strategy to search for long-duration gravitational-wave signals
• Digital Discovery of interferometric Gravitational Wave Detectors
• Efficient prescription to search for linear gravitational wave memory from hyperbolic black hole encounters and its application to the NANOGrav 12.5-year dataset
• How much spin wandering can continuous gravitational wave search algorithms handle?
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Study of statistical properties of hybrid statistic in coherent multi-detector compact binary coalescences Search
• Chirp mass based glitch identification in long duration gravitational wave transients
• Complete Catalog of Laser Locking Configurations for LISA
• Mass function of stellar black holes as revealed by the LIGO-Virgo-KAGRA observations
• A global analysis for searching neutrinos associated with the black holes merging gravitational wave events
• Effect of spin in binary neutron star mergers
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Limits on the Stochastic Gravitational Wave Background and Prospects for Single Source Detection with GRACE Follow-On
• Gravitational friction from d'Alembert's principle
• Experimental investigation of the limitations of polarisation optics for future gravitational wave detectors based on the polarisation Sagnac speedmeter
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• Could GRB170817A be really correlated to a NS-NS merging?
• Laser Interferometer in Presence of Scalar field on Gravitational Wave Background
• Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Mechanical Characterisation of Silicon for the ETpathfinder Test Masses
• Extremely High-Order Convergence in Simulations of Relativistic Stars
• Genetic-algorithm-optimized neural networks for gravitational wave classification
• Testing for a Random Walk Structure in the Frequency Evolution of a Tone in Noise
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Study of acceleration measurement in gravitational wave detection
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• High speed, high power 2D beam steering for mitigation of optomechanical parametric instability in gravitational wave detectors
• Architectural Optimization and Feature Learning for High-Dimensional Time Series Datasets
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• Relative calibration of the LIGO and Virgo detectors using astrophysical events from their third observing run
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Measurement of the central Galactic black hole by extremely large mass-ratio inspirals
• Overlap reduction function for gravitational wave detectors in an expanding Universe
• Banks of templates for directed and all-sky narrow-band searches of continuous gravitational waves from spinning neutron stars with several spindowns
• The quantum state of light in collective spontaneous emission
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
• A gating-and-inpainting perspective on GW150914 ringdown overtone: understanding the data analysis systematics
• Constraining the abundance of spinning deformed Galactic compact objects with continuous gravitational waves
• Statistically-informed deep learning for gravitational wave parameter estimation
• Experimental demonstration of frequency downconverted arm length stabilization for a future upgraded gravitational wave detector
• Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
• The Virgo Newtonian calibration system for the O4 observing run
• Resonant behavior and stability of a linear three-mirror cavity
• Doppler correlation-driven vetoes for the Frequency Hough analysis in continuous gravitational-wave searches
• Application of Non-Linear Noise Regression in the Virgo Detector
• Route to hyperchaos in quadratic optomechanics
• Scalable matched-filtering pipeline for gravitational-wave searches of compact binary mergers
• Astrophysical constraints on neutron star $f$-modes with a nonparametric equation of state representation
• Fighting Newtonian Noise with Gradient-Based Optimization at the Einstein Telescope
• Multivariate Time Series Clustering for Environmental State Characterization of Ground-Based Gravitational-Wave Detectors
• Constraining the Luminosity Function and Delay-Time Distribution of Short Gamma-Ray Bursts for Multimessenger Gravitational-Wave Detection Rate Estimation
• Lindblad estimation with fast and precise quantum control
• Imprints of an early matter-dominated era arising from dark matter dilution mechanism on cosmic string dynamics and gravitational wave signatures
• Target-based Optimization of Advanced Gravitational-Wave Detector Network Operations
• Electromagnetic Continuum Induced Nonlinearity
• Complementary signatures of $\alpha -$attractor inflation in CMB and cosmic string Gravitational Waves
• A ${\chi }^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences
• Searching for continuous gravitational waves from highly deformed compact objects with DECIGO
• Proto-neutron star oscillations including accretion flows
• Resonant amplification of multimessenger emission in rotating stellar core collapse
• Towards asteroseismology of neutron stars with physics-informed neural networks
• Constraining scalar-tensor theories from higher harmonics with GW230529
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• Axion Dark Matter Archaeology with Primordial Gravitational Waves
• Exploring future synergies for large-scale structure between gravitational waves and radio sources
• Development of a polarimetry method toward in-situ substrate birefringence characterization of ground-based gravitational wave detectors
• Modeling Relative Peak Times of Gravitational Wave Harmonics
• Prospects for High-Frequency Gravitational-Wave Detection with GEO600
• Binary black holes in the heat of merger
• Improved Binary Black Hole Search Discriminator from the Singular Value Decomposition of Non-Gaussian Noise Transients
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• A Gaussian process framework for testing general relativity with gravitational waves
• Can Big Black Holes Merge with the Smallest Black Holes?
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries
• Challenging a binary neutron star merger interpretation of GW230529
• Methods for Estimating Neutron Star Parameters using Multiple Mechanisms for Gravitational Wave Emission Associated with Pulsar Glitches
• Machine Learning Confirms GW231123 is a "Lite" Intermediate Mass Black Hole Merger
• Learning to detect continuous gravitational waves: an open data-analysis competition
• Probing cosmic strings via gravitational-wave lensing
• A comprehensive look into the accuracy of SpEC binary black hole waveforms
• Quasinormal modes from numerical relativity with Bayesian inference
• GW250114 reveals black hole horizon signatures
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Performance comparison of multi-detector detection statistics in targeted compact binary coalescence GW search
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Flexible Gravitational-Wave Parameter Estimation with Transformers
• Revisiting Singlet Fermion Dark Matter with a Scalar Portal: Connecting Higgs Phenomenology and Strong Electroweak Phase Transition
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Simulating first-order phase transition during inflation
• Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• Strain sensitivity enhancement in a Grover-Michelson interferometer
• Quantum speed limit as a sensitive probe of Planck-scale effects
• Parameter Estimation Precision with Geocentric Gravitational Wave Interferometers: Monochromatic Signals
• High-efficiency Electro-Optic Lens for radio frequency beam wavefront modulation for mode mismatch sensing
• Peak energy--Isotropic Luminosity Correlation and Jet Opening Angle Evolution in Swift-BAT Short GRBs with Soft Tail Emission
• Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• A Systematic Error in the Internal Friction Measurement of Coatings for Gravitational Waves Detectors
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• Investigation of Mechanical Properties of Cryogenically Treated Music Wire
• Multimessenger Analysis Strategy for Core-Collapse Supernova Search: Gravitational Waves and Low-energy Neutrinos
• Bounding dark charges on binary black holes using gravitational waves
• Probing Dark Matter Clumps, Strings and Domain Walls with Gravitational Wave Detectors
• Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
• APRIL: Auxiliary Physically-Redundant Information in Loss -- A physics-informed framework for parameter estimation with a gravitational-wave case study
• Detecting White Dwarf Binary Mergers with Gravitational Waves
• Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise
• Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
• Capability for detection of GW190521-like binary black holes with TianQin
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources
• Dynamical double black holes and their host cluster properties
• Global time-frequency search for stellar-mass binary black holes in LISA
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• $\kappa$-General-Relativity II: An Astrophysical Observable from a 2-Body system
• Observation of an Optical Spring in a Robustly Controlled Signal-Recycled Michelson Interferometer
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
• Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
• Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model
• Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
• Demonstration of a switchable damping system to allow low-noise operation of high-Q low-mass suspension systems
• Toward a Unified Understanding of the Dense Matter Equation of State
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Using machine learning to auto-tune chi-squared tests for gravitational wave searches
• Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
• Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
• GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform
• Demonstration of tilt sensing using a homodyne quadrature interferometric translational sensor
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector
• In situ substrate birefringence characterization in gravitational wave detectors using a heterodyne polarimetry method
• Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
• Hamiltonian normal forms for the post-Newtonian binary problem
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Very-High-Frequency Gravitational Waves from Multi-Monodromy Inflation
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference
• True and apparent motion of optomechanical resonators, with applications to feedback cooling of gravitational wave detector test masses
• Enhancing the significance of astrophysical events with multimessenger coincidences
• Constraints on r-modes and mountains on millisecond neutron stars in binary systems
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Probing the Neutrino Seesaw Scale with Gravitational Waves
• Hierarchical search for compact binary coalescences in the Advanced LIGO's first two observing runs
• Population Properties of Binary Black Holes with Eccentricity
• Hard thermal contributions to phase transition observables at NNLO
• Interferometric sensing of a commercial geophone
• Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
• Effects of local cosmic inhomogeneities on the gravitational wave event rate
• Cordierite-based optical resonators with extremely low thermal expansion
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• 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
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• Gravitational-wave astronomy requires population-informed parameter estimation
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• labrador: A domain-optimized machine-learning tool for gravitational wave inference
• Tests of scalar polarizations with multi-messenger events
• Deep searches for X-ray pulsations from Scorpius X-1 and Cygnus X-2 in support of continuous gravitational wave searches
• Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
• No model-independent evidence for a peak in binary black hole spin (mis)alignments
• Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
• $e^{+}{e}^{-}$ annihilation on the stochastic background of primordial gravitational waves with BKP18
• Efficient Evaluation of Gravitational Lensing Amplification Factors: A Deep Learning Framework
• Gravitational wave memory and quantum Michelson interferometer
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Unveiling gravitational waves from core-collapse supernovae with MUSE
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Evaluation of microseismic motion at the KAGRA site based on ocean wave data
• Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies
• SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Effect of the cosmological parameters on gravitational waves: general analysis
• Non canonical polarizations of Gravitational Waves
• Design of a tabletop interferometer with quantum amplification
• A Novel Search Technique for Low-Frequency Periodic Gravitational Waves
• Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
• Analysing one- and two-bit data to reduce memory requirements for F-statistic-based gravitational wave searches
• Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope
• Primordial black holes capture by stars and induced collapse to low-mass stellar black holes
• 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
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• Redshift factor and the small mass-ratio limit in binary black hole simulations
• Correlation analysis for isotropic stochastic gravitational wave backgrounds with maximally allowed polarization degrees
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
• Characterization of merging black holes with two precessing spins
• Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
• Multi-scale optimal control for Einstein Telescope active seismic isolation
• Gravitational waves from spinning neutron stars as not-quite-standard sirens
• Global Gravity Field Model from Taiji-1 Observations
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• Hot news on the phase structure of the SMEFT
• A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Model-agnostic gravitational-wave background characterization algorithm
• 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
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• The nuclear matter density functional under the nucleonic hypothesis
• Using tunable coherence for reaching micrometer coherence lengths and suppressing stray light in a power-recycled Michelson interferometer
• Gravity Induced Quantum Interference on Gravitational Wave Background
• An Order Statistics Post-Mortem on LIGO-Virgo GWTC-2 Events Analysed with Nested Sampling
• Time-dependent deflection reconstruction: new technique to search for gravitational waves with the cosmic microwave background
• Examining the Gap in the Chirp Mass Distribution of Binary Black Holes
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• Where are Gaia's small black holes?
• Reducing suspension control noise with interferometric sensors -- an experimental concept
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• Differentiating between sharp and smoother phase transitions in neutron stars
• Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Scalar-Induced Gravitational Waves in Palatini $f(R)$ Gravity
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Impact of facility timing and coordination for next-generation gravitational-wave detectors