Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

Abstract

Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is the method by which gravitational-wave data is used to infer the sources' astrophysical properties. We introduce a user-friendly Bayesian inference library for gravitational-wave astronomy, Bilby. This python code provides expert-level parameter estimation infrastructure with straightforward syntax and tools that facilitate use by beginners. It allows users to perform accurate and reliable gravitational-wave parameter estimation on both real, freely-available data from LIGO/Virgo, and simulated data. We provide a suite of examples for the analysis of compact binary mergers and other types of signal model including supernovae and the remnants of binary neutron star mergers. These examples illustrate how to change the signal model, how to implement new likelihood functions, and how to add new detectors. Bilby has additional functionality to do population studies using hierarchical Bayesian modelling. We provide an example in which we infer the shape of the black hole mass distribution from an ensemble of observations of binary black hole mergers.

Submitted for publication

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• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• Linear to circular conversion in the polarized radio emission of a magnetar
• Gravitational wave detection without boot straps: a Bayesian approach
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Cosmography with Standard Sirens from the Einstein Telescope
• Bayesian Time Delay Interferometry
• The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves
• Searching for quasi-periodic oscillations in astrophysical transients using Gaussian processes
• Gaussian Processes for Glitch-robust Gravitational-wave Astronomy
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Utilizing the null stream of the Einstein Telescope
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• The anti-aligned spin of GW191109: glitch mitigation and its implications
• Orbital eccentricity in a neutron star - black hole merger
• Is there a spectral turnover in the spin noise of millisecond pulsars?
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
• Improving Detection of Gravitational wave Microlensing Using Repeated Signals Induced by Strong Lensing
• Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories
• jetsimpy: A Highly Efficient Hydrodynamic Code for Gamma-ray Burst Afterglow
• Exploring gravitational-wave detection and parameter inference using Deep Learning methods
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• 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
• Constraining gravitational wave amplitude birefringence with GWTC-3
• Astrophysics and Nuclear Physics Informed Interactions in Dense Matter: Inclusion of PSR J0437-4715
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Pitfalls of periodograms: The non-stationarity bias in the analysis of quasi-periodic oscillations
• Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
• Hints of spin-orbit resonances in the binary black hole population
• Prospects for Taiji to detect a gravitational-wave background from cosmic strings
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• The reliability of the low-latency estimation of binary neutron star chirp mass
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Detection and estimation of the cosmic dipole with the Einstein Telescope and Cosmic Explorer
• Density estimation with Gaussian processes for gravitational-wave posteriors
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Identifying strongly lensed gravitational waves through their phase consistency
• Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Constrains on the electric charges of the binary black holes with GWTC-1 events
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• GW230529_181500: A Potential Primordial Binary Black Hole Merger in the Mass Gap
• Probing hadron-quark phase transition in twin stars using $f$-modes
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Mass$\unicode{x2013}$spin Re-Parameterization for Rapid Parameter Estimation of Inspiral Gravitational-Wave Signals
• Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Does the speed of gravitational waves depend on the source velocity?
• Spin Doctors: How to diagnose a hierarchical merger origin
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Tidal Disruption Events through the Lens of the Cooling Envelope Model
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• PSR~J1910$-$5959A: A rare gravitational laboratory for testing white dwarf models
• GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Incorporation of model accuracy in gravitational wave Bayesian inference
• A stochastic search for intermittent gravitational-wave backgrounds
• Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
• The astrophysical odds of GW151216
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?
• The birth mass function of neutron stars
• Gravitational wave constraints on non-birefringent dispersions of gravitational waves due to Lorentz violations with GWTC-3
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Footprints of population III stars in the gravitational-wave background
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
• Measuring quasi-normal mode amplitudes with misaligned binary black hole ringdowns
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Bayesian modelling of scattered light in the LIGO interferometers
• Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620
• GRB 220426A: A Thermal Radiation-Dominated Gamma-Ray Burst
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• Possible binary neutron star merger history of the primary of GW230529
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• Evidence of the pair instability gap from black hole masses
• Dark Stars and Gravitational Waves: Topical Review
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Detection of strong scattering close to the eclipse region of PSR B1957+20
• Uncovering dark matter density profiles in dwarf galaxies with graph neural networks
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• Searching for gravitationally lensed gamma-ray bursts with their afterglows
• Constraining the Gravitational-Wave Spectrum from Cosmological First-Order Phase Transitions Using Data from LIGO-Virgo First Three Observing Runs
• Orbital dynamics and extreme scattering event properties from long-term scintillation observations of PSR J1603-7202
• Parameter Estimation of Gravitational Waves with a Quantum Metropolis Algorithm
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• Energy-dependent intrinsic time delay of gamma-ray bursts on testing Lorentz invariance violation
• Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
• Glitch-induced pulse profile change of PSR J0742-2822 observed from the IAR
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• GLANCE -- Gravitational Lensing Authenticator using Non-Modelled Cross-Correlation Exploration of Gravitational Wave Signals
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Isolated pulsar population synthesis with simulation-based inference
• Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Microlensing bias on the detection of strong lensing gravitational wave
• ArchEnemy: Removing scattered-light glitches from gravitational wave data
• The False Alarms induced by Gaussian Noise in Gravitational Wave Detectors
• Inconsistent black hole kick estimates from gravitational-wave models
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• Memory Effect or Cosmic String? Classifying Gravitational-Wave Bursts with Bayesian Inference
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Analysis of the ionized interstellar medium and orbital dynamics of PSR~J1909-3744 using scintillation arcs
• Cautionary tales on heating-rate prescriptions in kilonovae
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Rapid localization of gravitational wave hosts with FIGARO
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• A matched-filter approach to radio variability and transients: searching for orphan afterglows in the VAST Pilot Survey
• Gravitational wave echoes search with combs
• The ultra narrow FRB20191107B, and the origins of FRB scattering
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Analysis of the subsolar-mass black hole candidate SSM200308 from the second part of the third observing run of Advanced LIGO-Virgo
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Constraining black-hole binary spin precession and nutation with sequential prior conditioning
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Prospects of calibrating afterglow modeling of short GRBs with gravitational wave inclination angle measurements and resolving the Hubble tension with a GW-GRB association event
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• The kinematic contribution to the cosmic number count dipole
• Reinvestigation of Fast Radio Burst Host Galaxy and Event Rate Density
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Realizing the potential of deep neural network for analyzing neutron star observables and dense matter equation of state
• Lorentz Invariance Violation from Gamma-Ray Bursts
• Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• Quasi-universal relations in the context of future neutron star detections
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Rotational and radio emission properties of PSR J0738-4042 over half a century
• Probing new fundamental fields with Extreme Mass Ratio Inspirals
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• On the initial spin period distribution of neutron stars
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
• Importance of eccentricities in parameter estimation of compact binary inspirals with decihertz gravitational-wave detectors
• Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak
• Bayesian $\mathcal{F}$-statistic-based parameter estimation of continuous gravitational waves from known pulsars
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Testing the robustness of simulation-based gravitational-wave population inference
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry
• An interference-based method for the detection of strongly lensed gravitational waves
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Unraveling the global behavior of equation of state by explicit finite nuclei constraints
• No evidence for a dip in the binary black hole mass spectrum
• Inferring Interference: Identifying a Perturbing Tertiary with Eccentric Gravitational Wave Burst Timing
• GPU-accelerated LISA parameter estimation with full time domain response
• Accelerated detection of the binary neutron star gravitational-wave background
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Millimeter emission from supermassive black hole coronae
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• Tests of weak equivalence principle with the gravitational wave signals in the LIGO-Virgo catalogue GWTC-1
• Identifying Strongly Lensed Gravitational Waves with the Third-generation Detectors
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Conditional Noise Deep Learning for Parameter Estimation of Gravitational Wave Events
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
• Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Constraining string cosmology with the gravitational-wave background using the NANOGrav 15-year data set
• Gaia EDR3 parallaxes of type I X-ray bursters and their implications on the models of type I X-ray bursts: a generic approach to the Gaia parallax zero-point and its uncertainty
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• Deep learning to detect gravitational waves from binary close encounters: Fast parameter estimation using normalizing flows
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
• Precessing Binary Black Holes as Better Dark Sirens
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Examining Lorentz invariance violation with three remarkable GRB photons
• Time delay interferometry with minimal null frequencies
• Bounds on the charge of the graviton using gravitational wave observations
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Convolutional Neural Networks for signal detection in real LIGO data
• Black Hole Gravitational Potential Enhanced Fallback Accretion onto the Nascent Lighter Compact Object: Tentative Evidence in the O3 Run Data of LIGO/Virgo
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Implementation of a generalized precession parameter in the RIFT parameter estimation algorithm
• Revealing Dark Matter's Role in Neutron Stars Anisotropy: A Bayesian Approach Using Multi-messenger Observations
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Detecting a Gravitational-Wave Background from Inflation with Null Energy Condition Violation: Prospects for Taiji
• Modelling Einstein cluster using Einasto profile
• Projections of the uncertainty on the compact binary population background using popstock
• Constraints on Brans-Dicke gravity from neutron star-black hole merger events using higher harmonics
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
• 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
• Inferring Binary Properties from Gravitational Wave Signals
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Inferring small neutron star spins with neutron star-black hole mergers
• Observability of spin precession in the presence of a black-hole remnant kick
• Simulation-based Inference for Gravitational-waves from Intermediate-Mass Binary Black Holes in Real Noise
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• Gravitational Wave emission in Binary Neutron Star early post-merger within a dark environment
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• Detection of disk-jet co-precession in a tidal disruption event
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
• Constraining the ellipticity and frequency of binary neutron star remnant via its gravitational-wave and electromagnetic radiations
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• A Joint Ranking Statistic for Multi-messenger Astronomical Searches with Gravitational Waves
• Searching for the spectral depolarisation of ASKAP one-off FRB sources
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Minimally-modeled search of higher multipole gravitational-wave radiation in compact binary coalescence
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Model-independent search for the quasinormal modes of gravitational wave echoes
• Tidal dissipation in binary neutron star inspirals from hyperon bulk viscosity: Phase modeling and parameter estimation bias
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Inferring properties of neutron stars born in short gamma-ray bursts with a plerion-like X-ray plateau
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• TESLA-X: An effective method to search for sub-threshold lensed gravitational waves with a targeted population model
• The Bulk Properties of Isolated Neutron Stars Inferred from the Gravitational Redshift Measurements
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Dynamical Measurement of Supermassive Black Hole Masses: QPE Timing Method
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Carpet-3 300 TeV Photon Event as an Evidence for Lorentz Violation
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Forecast Analysis of Astrophysical Stochastic Gravitational Wave Background beyond general relativity: A Case Study on Brans-Dicke Gravity
• Diffraction around caustics in gravitational wave lensing
• Vetting quark-star models with gravitational waves in the hierarchical Bayesian framework
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Unveiling a universal relationship between the f(R) parameter and neutron star properties
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• The directional isotropy of LIGO-Virgo binaries
• Surrogate models for lightcurves and photosphere properties of Type II supernovae
• Vacuum birefringence and the polarized X-ray emission from a radio magnetar
• Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Verification of the Black Hole Area Law with GW230814
• Upper limits on the temperature of inspiraling astrophysical black holes
• Optimized localization for gravitational-waves from merging binaries
• Probing black hole `charge' from the binary black hole inspiral
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• GRB 201104A: A "Repetitive" Short Gamma-Ray Burst?
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Potential impact of noise correlation in next-generation gravitational wave detectors
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• The origin of the coherent radio flash potentially associated with GRB 201006A
• Unveiling the existence of nontensorial gravitational-wave polarizations from individual supermassive black hole binaries with pulsar timing arrays
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Search for continuous gravitational waves from unknown neutron stars in binary systems with long orbital periods in O3 data
• Measuring the speed of gravity and the cosmic expansion with time delays between gravity and light from binary neutron stars
• Bayesian technique to combine independently-trained Machine-Learning models applied to direct dark matter detection
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• On non-detection of Gamma-Ray Bursts in three compact binary merger events detected by LIGO
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Bayesian WIMP detection with the Cherenkov Telescope Array
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Study of pulsar flux density and its variability with Parkes data archive
• Quantum Bayesian Inference with Renormalization for Gravitational Waves
• Parameter estimation of binary black holes in the endpoint of the up-down instability
• GW170814: Gravitational wave polarization analysis
• Joint inference for gravitational wave signals and glitches using a data-informed glitch model
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• Inferring the spins of merging black holes in the presence of data-quality issues
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• Testing beyond-Kerr spacetimes with GWTC-3
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Probing magneto-ionic microstructure towards the Vela pulsar using a prototype SKA-Low station
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• Unveiling the nature of the Einstein Probe transient EP 241021a
• Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
• The prospects of gravitational waves on constraining the anisotropy of the Universe
• Optimizing the low-latency localization of gravitational waves
• What to expect: kilonova light curve predictions via equation of state marginalization
• GW231123: Overlapping Gravitational Wave Signals?
• Searching for topological dark matter in LIGO data
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Is PSR J0514$-$4002E in a PBH-NS binary?
• Possible discrimination of black hole origins from the lensing rate of DECIGO and B-DECIGO sources
• Mergers of hairy black holes: Constraining topological couplings from entropy
• Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• Black hole information recovery from gravitational waves
• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
• A weakly-modeled search for compact binary coalescences in Einstein Telescope
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• A Bayesian Inference Framework for Gamma-Ray Burst Afterglow Properties
• Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Metric Assisted Stochastic Sampling (MASS) search for gravitational waves from binary black hole mergers
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Einstein@Home all-sky "bucket" search for continuous gravitational waves in LIGO O3 public data
• Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
• Expect the unexpected: augmented mixture models for black-hole-population studies
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• Gravitational waves from magnetorotational core-collapse supernovae using 3D GRMHD simulations: effect of rotation and magnetic fields
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• Accelerated inference of microlensed gravitational waves with machine learning
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Computing spectral shifts for Johannsen-Psaltis black holes
• Discovering gravitational waveform distortions from lensing: A deep dive into GW231123
• RRAT J2325-0530: A Rotating Radio Transient with an Atypical Waiting-time Distribution
• A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Probing chromatic onsets of gravitational wave overtones
• Integrating Quantum Algorithms with Gravitational-Wave Metrology for Enhanced Signal Detection
• The Detection Prospect of the Counter Jet Radiation in the Late Afterglow of GRB 170817A
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
• Methods for Estimating Neutron Star Parameters using Multiple Mechanisms for Gravitational Wave Emission Associated with Pulsar Glitches
• Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
• Constraining scalar-tensor theories from higher harmonics with GW230529
• Fermi-GBM Observations of GRB 210812A: Signatures of a Million Solar Mass Gravitational Lens
• SageNet: Fast Neural Network Emulation of the Stiff-amplified Gravitational Waves from Inflation
• Application of Non-Linear Noise Regression in the Virgo Detector
• Machine Learning Confirms GW231123 is a "Lite" Intermediate Mass Black Hole Merger
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Bayesian Framework to Follow-up Continuous Gravitational Wave Candidates from Deep Surveys
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• Statistical biases in parametrized searches for gravitational-wave polarizations
• The DESI DR1 Peculiar Velocity Survey: global zero-point and $H_0$ constraints
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• Challenging a binary neutron star merger interpretation of GW230529
• A Bayesian approach to time-domain Photonic Doppler Velocimetry
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Probing cosmic strings via gravitational-wave lensing
• Can Big Black Holes Merge with the Smallest Black Holes?
• Flexible Gravitational-Wave Parameter Estimation with Transformers
• A Gaussian process framework for testing general relativity with gravitational waves
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• First Overtone Mode in the Ringdown Signal of GW231028
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• The spin-orbit alignment hypothesis in millisecond pulsars
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Bayesian analysis of the complex singlet model with phase transition gravitational waves
• The search of higher multipole radiation in gravitational waves from compact binary coalescences by a minimally-modelled pipeline
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Characterization of merging black holes with two precessing spins
• Inferring the nuclear symmetry energy at supra saturation density from neutrino cooling
• Inferring binary black holes stellar progenitors with gravitational wave sources
• An Order Statistics Post-Mortem on LIGO-Virgo GWTC-2 Events Analysed with Nested Sampling
• GWCloud: a searchable repository for the creation and curation of gravitational-wave inference results
• Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
• Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
• Hybrid waveforms for precessing quasi-circular binary systems
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Impact of facility timing and coordination for next-generation gravitational-wave detectors
• A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences
• Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Graph-based Summary Statistics for Revealing the Stochastic Gravitational Wave Background in Pulsar Timing Arrays
• Mode changing in J1909$-$3744: the most precisely timed pulsar
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars : Spinning case
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
• High-frequency continuous gravitational waves searched in LIGO O3 public data with Einstein@Home
• Model-agnostic search of gravitational wave echoes in LVK data
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Across the Universe: GW231123 as a magnified and diffracted black hole merger
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Gravitational Wave Informed Inference of 21-cm Global Signal Parameters
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Bayesian Inference of Neutron Star Properties in $f(Q)$ Gravity Using NICER Observations
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Gravitational-wave astronomy requires population-informed parameter estimation
• labrador: A domain-optimized machine-learning tool for gravitational wave inference
• No model-independent evidence for a peak in binary black hole spin (mis)alignments
• Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin-Velocity Alignment
• Low-efficiency long gamma-ray bursts: A case study with AT2020blt
• Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies
• Stochastic gravitational wave background due to core collapse resulting in neutron stars
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• AthenaK simulations of the binary black hole merger GW150914
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data