GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$

Abstract

On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 is from a quasicircular binary inspiral, then the detected signal is consistent with the merger of two black holes with masses of $85_{-14}^{+21}{M}_{\odot }$ and $66_{-18}^{+17}{M}_{\odot }$ (90 % credible intervals). We infer that the primary black hole mass lies within the gap produced by (pulsational) pair-instability supernova processes, and has only a 0.32 % probability of being below $65M_{\odot }$. We calculate the mass of the remnant to be $142_{-16}^{+28}{M}_{\odot }$, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is $5.3_{-2.6}^{+2.4}$ Gpc, corresponding to a redshift of $0.82_{-0.34}^{+0.28}$. The inferred rate of mergers similar to GW190521 is $0.13_{-0.11}^{+0.30}{\mathrm{Gpc}}^{-3}{\mathrm{yr}}^{-1}$.

arXiv commentSupplementary Material at https://dcc.ligo.org/LIGO-P2000020/Public

References in corpus (105)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• Advanced LIGO
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• Tests of general relativity with GW150914
• The Nucleosynthetic Signature of Population III
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• Laser Interferometer Space Antenna
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Coalescing binary systems of compact objects to (post)$^{5/2}-Newtonian order. V. Spin Effects
• Pulsational Pair-Instability Supernovae
• A simple model of complete precessing black-hole-binary gravitational waveforms
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Pulsational pair instability as an explanation for the most luminous supernovae
• The PyCBC search for gravitational waves from compact binary coalescence
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
• FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
• Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
• Production of Intermediate-Mass Black Holes in Globular Clusters
• Matched filtering of gravitational waves from inspiraling compact binaries: Computational cost and template placement
• Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
• The SXS Collaboration catalog of binary black hole simulations
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• The promise of multi-band gravitational wave astronomy
• Surrogate models for precessing binary black hole simulations with unequal masses
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
• Testing the no-hair theorem with GW150914
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• A chi-squared time-frequency discriminator for gravitational wave detection
• Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
• New binary black hole mergers in the second observing run of Advanced LIGO and Advanced Virgo
• Intermediate mass black holes in AGN disks: I. Production & Growth
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties
• Are merging black holes born from stellar collapse or previous mergers?
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• Missing Link Found? --- The ``runaway'' path to supermassive black holes
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• Observational evidence for intermediate-mass black holes
• Merging black holes in young star clusters
• 2-OGC: Open Gravitational-wave Catalog of binary mergers from analysis of public Advanced LIGO and Virgo data
• The final spin from binary black holes in quasi-circular orbits
• Multiresolution techniques for the detection of gravitational-wave bursts
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• Detecting binary compact-object mergers with gravitational waves: Understanding and Improving the sensitivity of the PyCBC search
• Georgia Tech Catalog of Gravitational Waveforms
• Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
• Observational Black Hole Spectroscopy: A time-domain multimode analysis of GW150914
• Constraint Likelihood analysis for a network of gravitational wave detectors
• Including higher order multipoles in gravitational-wave models for precessing binary black holes
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• PyCBC Live: Rapid Detection of Gravitational Waves from Compact Binary Mergers
• Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
• Binary black holes in young star clusters: the impact of metallicity
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• Multiband gravitational-wave event rates and stellar physics
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Distinguishing short duration noise transients in LIGO data to improve the PyCBC search for gravitational waves from high mass binary black hole mergers
• Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
• Reconstructing the calibrated strain signal in the Advanced LIGO detectors
• Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes
• Detectability of Intermediate-Mass Black Holes in Multiband Gravitational Wave Astronomy
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• The second RIT binary black hole simulations catalog and its application to gravitational waves parameter estimation
• Summed Parallel Infinite Impulse Response (SPIIR) Filters For Low-Latency Gravitational Wave Detection
• Detecting Intermediate-Mass Ratio Inspirals From The Ground And Space
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• Tracking black hole kicks from gravitational wave observations
• Effectual gravitational-wave template banks for coalescing compact binaries using a hybrid placement algorithm
• Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
• Impact of Higher-order Modes on the Detection of Binary Black Hole Coalescences
• Search for Gravitational Waves from Intermediate Mass Binary Black Holes
• A method to estimate the significance of coincident gravitational-wave observations from compact binary coalescence
• Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run
• Hybrid geometric-random template placement algorithm for gravitational wave searches from compact binary coalescences
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• A wider look at the gravitational-wave transients from GWTC-1 using an unmodeled reconstruction method
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• Measuring Spin of the Remnant Black Hole from Maximum Amplitude
• Decoding the final state in binary black hole mergers

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• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• Gravitational tuning forks and hierarchical triple systems
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Parameter estimation of stellar-mass black hole binaries with LISA
• Impact of the wave-like nature of Proca stars on their gravitational-wave emission
• Constraining the Merger History of Primordial-Black-Hole Binaries from GWTC-3
• Dynamics of binary black holes in low-mass young star clusters
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Identifying when Precession can be Measured in Gravitational Waveforms
• Analog Schwarzschild black holes of Bose-Einstein condensates in a cavity: Quasinormal modes and quasibound states
• Simulations predict intermediate-mass black hole formation in globular clusters
• Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
• Core-Halo Mass Relation in Scalar Field Dark Matter Models and its Consequences for the Formation of Supermassive Black Holes
• Ultralight bosons for strong gravity applications from simple Standard Model extensions
• Thermodynamical topology of quantum BTZ black hole
• Search for black hole hyperbolic encounters with gravitational wave detectors
• Contracting and Expanding Binary Black Holes in 3D Low-Mass AGN Disks: The Importance of Separation
• Synchronised gravitational atoms from mergers of bosonic stars
• Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances
• Dynamical evolution of Population III stellar systems and the resulting binary statistics
• Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): Insights from the Dark Energy Survey Deep Fields
• Measuring the spins of heavy binary black holes
• Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• "Super-Kilonovae" from Massive Collapsars as Signatures of Black-Hole Birth in the Pair-instability Mass Gap
• Measuring binary black hole orbital-plane spin orientations
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Assessing the model waveform accuracy of gravitational waves
• Black hole spectroscopy horizons for current and future gravitational wave detectors
• Gas Assisted Binary Black Hole Formation in AGN Discs
• Generalised Hayward spacetimes: Geometry, matter and scalar quasinormal modes
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Fermion soliton stars
• Interstellar Gas Heating by Primordial Black Holes
• Impact of noise transients on low latency gravitational-wave event localisation
• Improved deep learning techniques in gravitational-wave data analysis
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• Evidence for the evolution of black hole mass function with redshift
• Thermonuclear Explosions and Accretion-induced Collapses of White Dwarfs in Active Galactic Nucleus Accretion Disks
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?
• New models with independent dynamical torsion and nonmetricity fields
• Primordial black hole mergers from three-body interactions
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• 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
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Event rate predictions of strongly lensed gravitational waves with detector networks and more realistic templates
• Bounds on GUP parameters from GW150914 and GW190521
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• The Importance of Priors on LIGO-Virgo Parameter Estimation: the Case of Primordial Black Holes
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Shadows, rings and optical appearance of a magnetically charged regular black hole illuminated by various accretion disks
• Isolated and dynamical black hole mergers with \texttt{B-POP}: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers
• On the Jacobi capture origin of binaries with applications to the Earth-Moon system and black holes in galactic nuclei
• Algorithm for TDI numerical simulation and sensitivity investigation
• Probing Extremal Gravitational-Wave Events with Coarse-Grained Likelihoods
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• Where intermediate-mass black holes could hide in the Galactic Centre: A full parameter study with the S2 orbit
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars
• Primordial Black Hole Dark Matter evaporating on the Neutrino Floor
• Microlensing of gravitational waves by dark matter structures
• Ringdown frequencies in black holes formed from precessing black-hole binaries
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
• Dancing in the dark: detecting a population of distant primordial black holes
• Inferring the gravitational wave memory for binary coalescence events
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• A Study of Primordial Very Massive Star Evolution
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• Looking for the parents of LIGO's black holes
• Mass ejection in failed supernovae: equation of state and neutrino loss dependence
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Black Hole Leftovers: The Remnant Population from Binary Black Hole Mergers
• Filling the Black Hole Mass Gap: Avoiding Pair Instability in Massive Stars through Addition of Non-Nuclear Energy
• How loud are echoes from exotic compact objects?
• Investigating the relation between gravitational wave tests of general relativity
• The Role of Outflow Feedback on Accretion of Compact Objects in Accretion Disk of Active Galactic Nuclei
• Observing an intermediate mass black hole GW190521 with minimal assumptions
• Could PBHs and secondary GWs have originated from squeezed initial states?
• Gauge transformation of scalar induced tensor perturbation during matter domination
• Echoes from Asymmetric Wormholes and Black Bounce
• Optimization of model independent gravitational wave search using machine learning
• GW190521: Search for Echoes due to Stimulated Hawking Radiation from Black Holes
• Spin Evolution of Stellar-mass Black Holes Embedded in AGN disks: Orbital Eccentricity Produces Retrograde Circumstellar Flows
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
• GW190521 formation via three-body encounters in young massive star clusters
• Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision
• Intermediate Mass Black Hole Seeds from Cosmic String Loops
• Ready-to-use analytic model for gravitational waves from a hierarchical triple with Kozai-Lidov oscillations
• Primordial black hole formation for an anisotropic perfect fluid: Initial conditions and estimation of the threshold
• Kerr black holes with synchronised axionic hair
• Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• The hydrodynamic evolution of binary black holes embedded within the vertically stratified disks of active galactic nuclei
• GW190521 from the Merger of Ultra-Dwarf Galaxies
• Head-on collisions of $\ell$-boson stars
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Dwarf AGNs from Variability for the Origins of Seeds (DAVOS): Intermediate-mass black hole demographics from optical synoptic surveys
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Massive binary black holes from Population II and III stars
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• Alternative possibility of GW190521: Gravitational waves from high-mass black hole-disk systems
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• The Tarantula Massive Binary Monitoring V. R 144: a wind-eclipsing binary with a total mass > 140 Msun
• Growth of stellar mass black holes in dense molecular clouds and GW190521
• Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• GW190814 follow-up with the optical telescope MeerLICHT
• GW190521: tracing imprints of spin-precession on the most massive black hole binary
• 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
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations
• Fermi gas and modified gravity
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Exact Formulas for Spherical Photon Orbits Around Kerr Black Holes
• Lithium abundance is a gravitational model dependent quantity
• GWSkyNet: a real-time classifier for public gravitational-wave candidates
• Transient glitch mitigation in Advanced LIGO data with $\text{glitschen}$
• Optical Emission Model for Binary Black Hole Merger Remnants Travelling through Discs of Active Galactic Nuclei
• Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
• High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap
• Sky localization of space-based gravitational wave detectors
• Intermediate-mass black holes and the fundamental plane of black hole accretion
• Efficient multi-timescale dynamics of precessing black-hole binaries
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions
• Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• Observable signatures of stellar-mass black holes in active galactic nuclei
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• Universal features of gravitational waves emitted by superkick binary black hole systems
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Is there an excess of black holes around $20M_{\odot }$? Optimising the complexity of population models with the use of reversible jump MCMC
• Shadow of regular black hole in scalar-tensor-vector gravity theory
• Gravitational Faraday rotation of gravitational waves by a Kerr black hole
• The multipolar structure of rotating boson stars
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• The emergence of diffused Gamma-Ray Burst afterglows from the disks of Active Galactic Nuclei
• Modified Gravity and the Black Hole Mass Gap
• Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates
• GRB 191019A: a short gamma-ray burst in disguise from the disk of an active galactic nucleus
• A flexible Gaussian process reconstruction method and the mass function of the coalescing binary black hole systems
• Modeling gravitational waves from exotic compact objects
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• Statistical study of a large and cleaned sample of ultraluminous and hyperluminous X-ray sources
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• Inspiralling compact objects with generic deformations
• Bayesian parameter estimation on boson-star binary signals with a coherent inspiral template and spin-dependent quadrupolar corrections
• A Stability Timescale for Non-Hierarchical Three-Body Systems
• Mapping the Likelihood of GW190521 with Diverse Mass and Spin Priors
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• The first five years of gravitational-wave astrophysics
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• Metric-affine gravity effects on terrestrial (exo-)planets profiles
• Search for neutrinos in coincidence with gravitational wave events from the LIGO-Virgo O3a Observing Run with the Super-Kamiokande detector
• Detecting the stochastic gravitational wave background with the TianQin detector
• Boson stars in Palatini $f(\mathcal{R})$ gravity
• Prompt Emission of Gamma-Ray Bursts in the High-density Environment of Active Galactic Nuclei Accretion Disks
• Two-Scalar Bose-Einstein Condensates: From Stars to Galaxies
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• Theory-agnostic framework for inspiral tests of general relativity with higher-harmonic gravitational waves
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Primordial black holes from an inflationary potential valley
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Establishing the Non-Primordial Origin of Black Hole-Neutron Star Mergers
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Impact of a Midband Gravitational Wave Experiment On Detectability of Cosmological Stochastic Gravitational Wave Backgrounds
• "Conserved charges" of the Bondi-Metzner-Sachs algebra in the Brans-Dicke theory
• Utilizing the null stream of the Einstein Telescope
• Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
• Inferring spin tilts at formation from gravitational wave observations of binary black holes: Interfacing precession-averaged and orbit-averaged spin evolution
• GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications
• Binary black hole mergers from merged stars in the Galactic field
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Constraining a companion of the galactic center black hole, Sgr A*
• Extended phase-space symplectic-like integrators for coherent post-Newtonian Euler-Lagrange equations
• Constraining gravitational wave amplitude birefringence with GWTC-3
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Overcharging a Reissner-Nordström Taub-NUT regular black hole
• Hints of spin-orbit resonances in the binary black hole population
• Gravitational Waveform and Polarization from Binary Black Hole Inspiral in Dynamical Chern-Simons Gravity: From Generation to Propagation
• Jupiter and jovian (exo)-planets in Palatini $f(\bar{R})$ gravity
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• The gravitational capture of compact objects by massive black holes
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Biases in estimates of black hole kicks from the spin distribution of binary black holes
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Anomalies in the gravitational recoil of eccentric black-hole mergers with unequal mass ratios
• Pulsational pair-instability and the mass gap of Population III Black Holes: Effects of overshooting
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• Black hole event horizons are cosmologically coupled
• Distance and age of the massive stellar cluster Westerlund 1. I. Parallax method using Gaia-EDR3
• Testing the nature of dark compact objects with gravitational waves
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Frequency- and polarization-dependent lensing of gravitational waves in strong gravitational fields
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Mapping the Outcomes of Stellar Evolution in the Disks of Active Galactic Nuclei
• An elusive dark central mass in the globular cluster M4
• Improving the Robustness of the Advanced LIGO Detectors to Earthquakes
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds
• Electromagnetic emission from axionic boson star collisions
• Energy Extraction via Magnetic Reconnection in Konoplya-Rezzolla-Zhidenko Parametrized Black Holes
• Disc Novae: Thermodynamics of Gas Assisted Binary Black Hole Formation in AGN Discs
• Fundamental physics using the temporal gravitational wave background
• The Multi-mode Acoustic Gravitational Wave Experiment: MAGE
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• Binary black hole mergers from young massive and open clusters: comparison to GWTC-2 gravitational wave data
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Can we detect a supertranslated black hole?
• Interacting Kilonovae: Long-lasting Electromagnetic Counterparts to Binary Mergers in the Accretion Disks of Active Galactic Nuclei
• The Galactic Underworld: The spatial distribution of compact remnants
• Analyzing black-hole ringdowns II: data conditioning
• Impacts of Jets and Winds From Primordial Black Holes
• Post-merger chirps from binary black holes as probes of the final black-hole horizon
• Merging binary black holes formed through double-core evolution
• Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• MOCCA-SURVEY Database II -- Properties of Intermediate Mass Black Holes escaping from star clusters
• GW190521 formation scenarios via relativistic accretion
• Relaxing CMB bounds on Primordial Black Holes: the role of ionization fronts
• High-Precision Ringdown Surrogate Model for Non-Precessing Binary Black Holes
• Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Bondi-Hoyle-Lyttleton accretion onto a rotating black hole with ultralight scalar hair
• Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
• Implications of recoil kicks for black hole mergers from LIGO/Virgo catalogs
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Using supervised learning algorithms as a follow-up method in the search of gravitational waves from core-collapse supernovae
• Active platform stabilisation with a 6D seismometer
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• Iterative extraction of overtones from black hole ringdown
• Spin Doctors: How to diagnose a hierarchical merger origin
• Lensing rates of gravitational wave signals displaying beat patterns detectable by DECIGO and B-DECIGO
• $\mu$-distortion around stupendously large primordial black holes
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Compact Binary Merger Rate in Dark-Matter Spikes
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
• Multi-messenger Gravitational Lensing
• Angular Resolution of the Search for Anisotropic Stochastic Gravitational-Wave Background with Terrestrial Gravitational-Wave Detectors
• Fixing the dynamical evolution of self-interacting vector fields
• Measuring deviations from the Kerr geometry with black hole ringdown
• Detectability of Primordial Black Hole Binaries at High Redshift
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• Linear vs. nonlinear modeling of black hole ringdowns
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• 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
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Next-to-leading order spin-orbit effects in the equations of motion, energy loss and phase evolution of binaries of compact bodies in the effective field theory approach
• Improved inspiral-merger-ringdown model for BBHs on elliptical orbits
• Dark Stars and Gravitational Waves: Topical Review
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big Bang
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Evidence of the pair instability gap from black hole masses
• Learning orbital dynamics of binary black hole systems from gravitational wave measurements
• A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• Spin-induced scalarization and magnetic fields
• Hunting intermediate-mass black holes with LISA binary radial velocity measurements
• Production of PBHs from inflaton structure
• Using LSST Microlensing to Constrain Dark Compact Objects in Spherical and Disk Configurations
• Distinguishing the impact and signature of black holes from different origins in early cosmic history
• A general relativistic estimation of the black hole mass-to-distance ratio at the core of TXS 2226-184
• Fundamental Tone and Overtones of Quasinormal Modes in Ringdown Gravitational Waves: A Detailed Study in Black Hole Perturbation
• Energy-conserving integrator for conservative Hamiltonian systems with ten-dimensional phase space
• Existence of Zero-damped Quasinormal Frequencies for Nearly Extremal Black Holes
• One to many: comparing single gravitational-wave events to astrophysical populations
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Planetary seismology as a test of modified gravity proposals
• Observational limits on the rate of radiation-driven binary black hole capture events
• Giant planet formation in Palatini gravity
• A GPU-accelerated semi-coherent hierarchical search for stellar-mass binary inspiral signals in LISA
• Enhance Primordial Black Hole Abundance through the Non-linear Processes around Bounce Point
• Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• Parameter control for eccentric, precessing binary black hole simulations with SpEC
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Displacement memory effect near the horizon of black holes
• The implications of stochastic gas torques for asymmetric binaries in the LISA band
• Non-homogeneous exoplanets in metric-affine gravity
• The central black hole in the dwarf spheroidal galaxy Leo I Not supermassive, at most an intermediate-mass candidate
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• Quasinormal modes of slowly-spinning horizonless compact objects
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Spectroscopy for asymmetric binary black hole mergers
• Propagation of GRB Relativistic Jets in AGN Disks and Its Implication for GRB Detection
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Gravitational wave peak luminosity model for precessing binary black holes
• Dynamical Formation Scenarios for GW190521 and Prospects for Decihertz Gravitational-Wave Astronomy with GW190521-Like Binaries
• Radii of spherical photon orbits around Kerr-Newman black holes
• On the Tidal Capture of White Dwarfs by Intermediate-mass Black Holes in Dense Stellar Environments
• Simulation-based inference of black hole ringdowns in the time domain
• Central kinematics of the Galactic globular cluster M80
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• 2MASX J00423991+3017515: An offset active galactic nucleus in an interacting system
• Eccentricity estimation from initial data for Numerical Relativity Simulations
• Premature Black Hole Death of Population III Stars by Dark Matter
• What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Population properties of neutron stars in the coalescing compact binaries
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Constraining hierarchical mergers of binary black holes detectable with LIGO-Virgo
• Detectability of gravitational higher order modes in the third-generation era
• Resolving the Ultra-Luminous X-ray Sources in the Ly$\alpha$ Emitting Galaxy Haro 11
• Constraining black-hole binary spin precession and nutation with sequential prior conditioning
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• The imprint of superradiance on hierarchical black hole mergers
• Hypercritical accretion during common envelopes in triples leading to binary black holes in the pair-instability-supernova mass gap
• Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Central X-ray point-sources found to be abundant in low-mass, late-type galaxies predicted to contain an intermediate-mass black hole
• Eccentricity enables the earliest warning and localization of gravitational waves with ground-based detectors
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Horndeski fermion-boson stars
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Source localizations with the network of space-based gravitational wave detectors
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Outliers in the LIGO Black Hole Mass Function from Coagulation in Dense Clusters
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Method for detecting highly-eccentric binaries with a gravitational wave burst search
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• Efficient simulations of high-spin black holes with a new gauge
• A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak
• Motion of test particle in rotating boson star
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• Dictionary learning: a novel approach to detecting binary black holes in the presence of Galactic noise with LISA
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
• McFACTS II: Mass Ratio--Effective Spin Relationship of Black Hole Mergers in the AGN Channel
• Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
• Inferring Interference: Identifying a Perturbing Tertiary with Eccentric Gravitational Wave Burst Timing
• Detection of gravitational wave mixed polarization with single space-based detectors
• High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
• Extending superposed harmonic initial data to higher spin
• Light Rings around Five Dimensional Stationary Black Holes and Naked Singularities
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Swift X-ray Follow-Up Observations of Gravitational Wave and High-Energy Neutrino Coincident Signals
• Investigating the shadows of new regular black holes with a Minkowski core: Effects of spherical accretion and core type differences
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Dwarf AGNs from Variability for the Origins of Seeds (DAVOS): Optical Variability of Broad-line Dwarf AGNs from the Zwicky Transient Facility
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
• False positives for gravitational lensing: the gravitational-wave perspective
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field toy model
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Identifying Strongly Lensed Gravitational Waves with the Third-generation Detectors
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Applications of the close-limit approximation: horizonless compact objects and scalar fields
• Distortion of Gravitational-wave Signals by Astrophysical Environments
• Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
• Intermediate-mass ratio inspirals in merging elliptical galaxies
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Multimessenger hierarchical triple merger gravitational-wave event pair GW190514-GW190521 inside AGN J124942.3 + 344929
• Contribution of Flares from Tidal Disruption of Stars to high-redshift AGN
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• Core Noise Requirements, and GW Sensitivities of AMIGO
• Observational Properties of Thermal Emission from Relativistic Jets Embedded in AGN Disks
• Improving the stability of frequency dependent squeezing with bichromatic control of filter cavity length, alignment and incident beam pointing
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Primordial Black-Hole-Based Pathways to Little Red Dots
• Gamma rays from dark matter spikes in EAGLE simulations
• Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Wavelet-based tools to analyze, filter, and reconstruct transient gravitational-wave signals
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Primordial Black Hole Production in Natural and Hilltop Inflation
• Reconstruction of binary black hole harmonics in LIGO using deep learning
• Astrophysics with the Laser Interferometer Space Antenna
• Quantum manipulation of a two-level mechanical system
• Navigating Unknowns: Deep Learning Robustness for Gravitational Wave Signal Reconstruction
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Fate of initially bound timelike geodesics in spherical boson stars
• Unexpected LIGO events and the Mirror World
• Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
• Minimally-modeled search of higher multipole gravitational-wave radiation in compact binary coalescence
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Possibility of Primordial black holes Collision with Earth and the Consequences
• Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
• Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Modified Gravitation Theory (MOG) and the aLIGO GW190521 Gravitational Wave Event
• Detecting sublunar-mass primordial black holes with the Earth-Moon binary system
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Probing the large-scale structure of the universe through gravitational-wave observations
• Can Primordial Black Holes form in the Standard Model ?
• A search for intermediate-mass black holes in compact stellar systems through optical emissions from tidal disruption events
• CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
• Detection Landscape in the Deci-Hertz Gravitational-Wave Spectrum
• The Multiband Emission of the two-component Gamma-Ray Burst jet influenced by progenitor winds within the Accretion Disk of Active Galactic Nuclei
• Theory-agnostic searches for non-gravitational modes in black hole ringdown
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Black Hole Merger Rates in AGN: contribution from gas-captured binaries
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Recent LIGO-Virgo discoveries
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
• Probing black hole `charge' from the binary black hole inspiral
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
• Hawking Radiation Signatures from Primordial Black Holes Transiting the Inner Solar System: Prospects for Detection
• Relativistic Effects on Triple Black Holes: Burrau's Problem Revisited
• Cylindrical black hole solutions in $f(\mathcal{R})$ and $f(\mathcal{R},\mathcal{A},A^{\mu \nu }{A}_{\mu \nu })$ modified gravity
• Numerical-relativity surrogate modeling with nearly extremal black-hole spins
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• Probing eccentric higher-order modes through an effective chirp mass model
• Optimized localization for gravitational-waves from merging binaries
• Multi-messenger cosmology of new physics
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
• Charged Black Holes in Einsteinian Quartic Gravity
• 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
• Impacts of the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ reaction rate on ${}^{56}\mathrm{Ni}$ nucleosynthesis in pair-instability supernovae
• Shadowless rapidly rotating yet not ultraspinning Kerr-AdS${}_4$ and Kerr-Newman-AdS${}_4$ black holes
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Identifying intermediate mass binary black hole mergers in AGN disks using LISA
• Gravitational wave signals from long lasting binary-single black hole encounters
• Not all roads lead to merger: AGN disc properties influence the interactions of highly unequal mass black holes
• All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• GW170814: Gravitational wave polarization analysis
• Investigation of crackling noise in the vibration isolation systems of the KAGRA gravitational wave detector
• Black Holes LIGO/Virgo Domination and Single-lined Binaries with a Black Hole Candidate Component
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• Prospects for estimating parameters from gravitational waves of superspinar binaries
• Isotropic cosmological model with aetherically active axionic dark matter
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• Weighing the Darkness III: How Gaia Could, but Probably Won't, Astrometrically Detect Free-Floating Black Holes
• GW231123: Overlapping Gravitational Wave Signals?
• Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Formation of a Bose Star in a Rotating Cloud
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Broadband X-ray spectral analysis of the ULX NGC 1313\,X-1 using JeTCAF: Origin of the ULX bubble
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Phantom BTZ black holes
• Quantum sensors with matter waves for GW observation
• Searching for topological dark matter in LIGO data
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Observable signature of magnetic tidal coupling in hierarchical triple systems
• Discovering gravitational waveform distortions from lensing: A deep dive into GW231123
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• Gravitational-wave bursts from spin-precessing black holes in binary systems
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• Chirp mass based glitch identification in long duration gravitational wave transients
• A nonparametric method to assess significance of events in search for gravitational waves with false discovery rate
• Variability as a new discovery channel for Intermediate-Mass Black Holes in the Time Domain Era
• Laser Interferometer in Presence of Scalar field on Gravitational Wave Background
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Detectability of Massive Boson Stars using Gravitational Waves from Fundamental Oscillations
• Effects of modified gravity on microscopic properties and cooling timescale of white dwarfs
• Binary black holes in magnetized AGN disks
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Is GW190521 a gravitational wave echo of wormhole remnant from another universe?
• Tachyonic Instability of Reissner-Nordström-Melvin Black Holes in Einstein-Maxwell-Scalar Theory
• Linear momentum flux from inspiralling compact binaries in quasi-elliptical orbits at 2.5 Post-Newtonian order
• Arm-Locking Frequency Noise Suppression for Astronomical Middle-Frequency Interferometric Gravitational Wave Observatory
• Space-based Gravitational Wave Observatories
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• A Mass-Shell Model of Compact Binary Coalescence
• First Overtone Mode in the Ringdown Signal of GW231028
• Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
• Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Spectral study of X-ray sources in some galaxies recently observed by Chandra
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Testing the Quantum Equivalence Principle with Gravitational Waves
• Fundamental oscillations as a tool to distinguish boson stars from neutron stars and black holes
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Gravitational signatures beyond Newton: exploring hierarchical three-body dynamics
• Can dark-matter Q-balls grow to the mass gap masses?
• Partial tidal disruption of White Dwarfs in off-equatorial orbits around Kerr black holes
• An accurate model for the primordial black hole mass distribution from a peak in the power spectrum
• The Steady State of Intermediate-Mass Black Holes Near a Supermassive Black Hole
• Evidence of large recoil velocity from a black hole merger signal
• A gating-and-inpainting perspective on GW150914 ringdown overtone: understanding the data analysis systematics
• Relativistic Coulomb Screening in Pulsational Pair Instability Supernovae
• Perturbative solution of the Einstein Constraints with Spin and Momentum Far Away From a Binary Source in the Bowen-York formalism
• Lensing by primordial black holes: constraints from gravitational wave observations
• Challenging theories of gravitation: dark matter, compact objects and gravitational waves
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• Gravitational-wave matched filtering on a quantum computer
• Hierarchical Merger of Primordial Black Holes in Dwarf Galaxies
• The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
• Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries
• Machine Learning Confirms GW231123 is a "Lite" Intermediate Mass Black Hole Merger
• Assessment of Effective-One-Body Radiation Reactions for Generic Planar Orbits
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Black holes
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• An expanded ultraluminous X-ray source catalogue
• Gravitational radiation with kinetic recoil
• Distinguishing between dark-matter interactions with gravitational-wave detectors
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Proposed large scale monolithic fused silica mirror suspension for 3rd generation gravitational wave detectors
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Black hole or Gravastar? The GW190521 case
• Gravitational wave astronomy: astrophysical and cosmological inferences
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits
• Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
• Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
• Shadows and photon spheres of static black holes embedded in a Dehnen-(1,4,5/2)-type dark matter halo with a quintessential field
• Phase transition for a black hole with matter fields and the relation with the Lyapunov exponent
• The next generation: Impact of high-order analytical information on effective one body waveform models for noncircularized, spin-aligned black hole binaries
• Homothetic Killing horizons in generic Vaidya spacetimes
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Exceptionality of exceptional gravitational-wave events
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• A Multi-Mission Catalogue of Ultraluminous X-ray Source Candidates
• The Gravity of Classical Fields: And Its Effect on the Dynamics of Gravitational Systems
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• Gravitational Wave Signatures of Quasi-Periodic Eruptions: LISA Detection Prospects for RX J1301.9+2747
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Black-hole ringdown with templates capturing spin precession: A reanalysis of GW190521
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• Global time-frequency search for stellar-mass binary black holes in LISA
• GWCloud: a searchable repository for the creation and curation of gravitational-wave inference results
• Description and Application of the Surfing Effect
• A template-free approach for waveform extraction of gravitational wave events
• Observing GW190521-like binary black holes and their environment with LISA
• 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
• Exploiting Newton-factorized, 2PN-accurate, waveform multipoles in effective-one-body models for spin-aligned noncircularized binaries
• Search of Intermediate Mass Black Holes at Low Redshift with Intra-night Variability
• Black Hole merger rates in the first billion years in light of JWST data
• The Role of High-mass Stellar Binaries in the Formation of High-mass Black Holes in Dense Star Clusters
• Inferring binary black holes stellar progenitors with gravitational wave sources
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Tidal disruptions of close white dwarf binaries by intermediate mass black holes
• Sequence modeling of higher-order wave modes of binary black hole mergers
• Capability for detection of GW190521-like binary black holes with TianQin
• gSeaGen code by KM3NeT: an efficient tool to propagate muons simulated with CORSIKA
• Dynamical double black holes and their host cluster properties
• Ultralight bosonic dark matter in white dwarfs and potential observational consequences