Astrophysics with the Laser Interferometer Space Antenna

Abstract

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA's first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultracompact stellar-mass binaries, massive black hole binaries, and extreme or intermediate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.

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• Secular evolution of compact binaries near massive black holes: gravitational wave sources and other exotica
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• Chaotic cold accretion onto black holes
• Evolution of massive binary black holes
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• Accretion during the merger of supermassive black holes
• Stellar disk in the galactic center -- a remnant of a dense accretion disk?
• Faint Thermonuclear Supernovae from AM Canum Venaticorum Binaries
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• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function at z < 0.06
• Formation of the first three gravitational-wave observations through isolated binary evolution
• A gaseous metal disk around a white dwarf
• The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
• A unified model for tidal disruption events
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• Pōniuā'ena: A Luminous $z=7.5$ Quasar Hosting a 1.5 Billion Solar Mass Black Hole
• Magnetic White Dwarfs
• The distribution and cosmic evolution of massive black hole spins
• Self-regulated growth of supermassive black holes by a dual jet/heating AGN feedback mechanism: methods, tests and implications for cosmological simulations
• The Formation of Population III Binaries from Cosmological Initial Conditions
• Intermediate mass black holes in AGN disks: I. Production & Growth
• Ancient planetary systems are orbiting a large fraction of white dwarf stars
• The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
• On the formation and evolution of black-hole binaries
• Starbursts near supermassive black holes: young stars in the Galactic Center, and gravitational waves in LISA band
• Formation of the First Stars by Accretion
• The Kozai Mechanism and the Evolution of Binary Supermassive Black Holes
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• Steepest growth of the power spectrum and primordial black holes
• Modeling the Metallicity Distribution of Globular Clusters
• Cosmological black hole spin evolution by mergers and accretion
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• The Formation of Eccentric Compact Binary Inspirals and the Role of Gravitational Wave Emission in Binary-Single Stellar Encounters
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• Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (II) Ringdown
• The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs
• The evolution of massive black hole seeds
• Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties
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• Multiband lightcurves of tidal disruption events
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• A systematic search for close supermassive black hole binaries in the Catalina Real-Time Transient Survey
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• A synthesis model for AGN evolution: supermassive black holes growth and feedback modes
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• Accelerating Compact Object Mergers in Triple Systems with the Kozai Resonance: A Mechanism for "Prompt" Type Ia Supernovae, Gamma-Ray Bursts, and Other Exotica
• Formation of the first nuclear clusters and massive black holes at high redshift
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• An ALMA [CII] survey of 27 quasars at z>5.94
• Alignment of the spins of supermassive black holes prior to coalescence
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• Long Term Evolution of Massive Black Hole Binaries
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• On the formation history of Galactic double neutron stars
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• False periodicities in quasar time-domain surveys
• The effect of the metallicity-specific star formation history on double compact object mergers
• The Astrophysics of Nanohertz Gravitational Waves
• Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
• Distinguishing Spin-Aligned and Isotropic Black Hole Populations With Gravitational Waves
• High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
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• Mass Transfer between Double White Dwarfs
• The Evolution of Black Hole Mass and Spin in Active Galactic Nuclei
• Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars
• B-Mode contamination by synchrotron emission from 3-years WMAP data
• Post-common-envelope binaries from SDSS. IX: Constraining the common-envelope efficiency
• Massive Black Hole Binary Evolution
• Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum
• Event rate estimates for LISA extreme mass ratio capture sources
• High-redshift clumpy discs and bulges in cosmological simulations
• The Afterglow of Massive Black Hole Coalescence
• A Bright Year for Tidal Disruptions?
• The impact of angular momentum on black hole accretion rates in simulations of galaxy formation
• Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds
• The Dynamical Evolution of Stellar Black Holes in Globular Clusters
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Observational evidence for intermediate-mass black holes
• "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
• Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
• Evidence for Warped Disks of Young Stars in the Galactic Center
• Accretion into the Central Cavity of a Circumbinary Disk
• Massive black hole binaries from runaway collisions: the impact of metallicity
• The Assembly of Supermassive Black Holes at High Redshifts
• The astrophysical gravitational wave stochastic background
• Pulsar Jets: Implications for Neutron Star Kicks and Initial Spins
• A Young White Dwarf Companion to Pulsar 1620-26: Evidence for Early Planet Formation
• Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
• Head-on collisions of white dwarfs in triple systems could explain type Ia supernova
• Discovery of a Candidate Black Hole - Giant Star Binary System in the Galactic Field
• Asymmetries in core-collapse supernovae from maps of radioactive ${}^{44}$Ti in CassiopeiaA
• What is the Highest Plausible Redshift of Luminous Quasars?
• Supermassive black hole binaries in gaseous and stellar circumnuclear discs: orbital dynamics and gas accretion
• The cosmic evolution of massive black holes in the Horizon-AGN simulation
• A New Empirical Model for the Structural Analysis of Early-type Galaxies and a Critical Review of the Nuker Model
• The origins of massive black holes
• Short-period AM CVn systems as optical, X-ray and gravitational wave sources
• Merging black holes in young star clusters
• Stellar-mass black holes in star clusters: implications for gravitational wave radiation
• BPASS predictions for Binary Black-Hole Mergers
• Massive perturber-driven interactions of stars with a massive black hole
• The evolution of massive black holes and their spins in their galactic hosts
• Post-common-envelope binaries from SDSS. XI: The white dwarf mass distributions of CVs and pre-CVs
• Rotational mixing in massive binaries: detached short-period systems
• Galactic distribution of merging neutron stars and black holes - prospects for short GRB progenitors and LIGO/VIRGO
• The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
• HST STIS spectroscopy of the triple nucleus of M31: two nested disks in Keplerian rotation around a Supermassive Black Hole
• Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter
• Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries
• Multi-Dimensional Simulations of the Accretion-Induced Collapse of White Dwarfs to Neutron Stars
• A Population of Short-Period Variable Quasars from PTF as Supermassive Black Hole Binary Candidates
• Fluctuations in the High-Redshift Lyman-Werner Background: Close Halo Pairs as the Origin of Supermassive Black Holes
• An AMR Study of the Common Envelope Phase of Binary Evolution
• Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters
• Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
• Direct Formation of Supermassive Black Holes via Multi-Scale Gas Inflows in Galaxy Mergers
• The DRAGON simulations: globular cluster evolution with a million stars
• Accelerating NBODY6 with Graphics Processing Units
• Gravitational torque-driven black hole growth and feedback in cosmological simulations
• The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO
• Can Supermassive Black Holes Form in Metal-Enriched High-Redshift Protogalaxies ?
• Clustering of Low-Redshift (z <= 2.2) Quasars from the Sloan Digital Sky Survey
• Quasar Quartet Embedded in Giant Nebula Reveals Rare Massive Structure in Distant Universe
• New physical insights about Tidal Disruption Events from a comprehensive observational inventory at X-ray wavelengths
• Matching matched filtering with deep networks in gravitational-wave astronomy
• Four-Body Effects in Globular Cluster Black Hole Coalescence
• Two stellar-mass black holes in the globular cluster M22
• Regular Black Hole Metric with Three Constants of Motion
• Measuring the Spins of Accreting Black Holes
• A black hole in a globular cluster
• Black-hole binaries, gravitational waves, and numerical relativity
• Tidal disruption and ignition of white dwarfs by moderately massive black holes
• MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
• Ubiquitous seeding of supermassive black holes by direct collapse
• Did NANOGrav see a signal from primordial black hole formation?
• Migration Traps in Disks Around Supermassive Black Holes
• Runaway collisions in young star clusters. II. Numerical results
• Dark matter distributions around massive black holes: A general relativistic analysis
• Ejection of Supermassive Black Holes from Galaxy Cores
• Supermassive Stars in Quasar Disks
• Inflationary primordial black holes for the LIGO gravitational wave events and pulsar timing array experiments
• Resonant relaxation near a massive black hole: the stellar distribution and gravitational wave sources
• Black holes in galaxies: environmental impact on gravitational-wave generation and propagation
• A recoiling supermassive black hole in the quasar SDSSJ092712.65+294344.0?
• Thermal Stability of White Dwarfs Accreting Hydrogen-rich Matter and Progenitors of Type Ia Supernovae
• Expected properties of the first gravitational wave signal detected with pulsar timing arrays
• GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
• A Large Systematic Search for Recoiling and Close Supermassive Binary Black Holes
• Reconstructing the spectral shape of a stochastic gravitational wave background with LISA
• The spin of the second-born black hole in coalescing binary black holes
• NBODY6++GPU: Ready for the gravitational million-body problem
• Fossil HII Regions: Self-Limiting Star Formation at High Redshift
• Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
• Massive Black Hole Binary Mergers in Dynamical Galactic Environments
• Hyper-Eddington accretion flows onto massive black holes
• The final spin from binary black holes in quasi-circular orbits
• Surface Detonations in Double Degenerate Binary Systems Triggered by Accretion Stream Instabilities
• Relativistic Measurements from Timing the Binary Pulsar PSR B1913+16
• Hydrodynamics of circumbinary accretion: Angular momentum transfer and binary orbital evolution
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• Black hole evolution: I. Supernova-regulated black hole growth
• Blossoms from black hole seeds: properties and early growth regulated by supernova feedback
• Spin orientations of merging black holes formed from the evolution of stellar binaries
• Timing the starburst-AGN connection
• The Fast, Luminous Ultraviolet Transient AT2018cow: Extreme Supernova, or Disruption of a Star by an Intermediate-Mass Black Hole?
• The dynamical evolution of massive black hole binaries - II. Self-consistent N-body integrations
• Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
• Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters
• Formation of millisecond pulsars with CO white dwarf companions - II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions
• A log-quadratic relation for predicting supermassive black hole masses from the host bulge Sersic index
• Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections
• Black hole mergers and blue stragglers from hierarchical triples formed in globular clusters
• Know Your Neighborhood: A Detailed Model Atmosphere Analysis of Nearby White Dwarfs
• Efficient Merger of Binary Supermassive Black Holes in Merging Galaxies
• Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits
• Gravitational waves induced by scalar perturbations as probes of the small-scale primordial spectrum
• Spectral energy distributions of selfgravitating QSO discs
• Relativistic Dynamics and Extreme Mass Ratio Inspirals
• Formation of massive black holes in rapidly growing pre-galactic gas clouds
• On the final spin from the coalescence of two black holes
• Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
• A New Sample of (Wandering) Massive Black Holes in Dwarf Galaxies from High Resolution Radio Observations
• Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation
• Chasing highly obscured QSOs in the COSMOS field
• Interaction of massive black hole binaries with their stellar environment: I. Ejection of hypervelocity stars
• Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations
• Gravitational waves at interferometer scales and primordial black holes in axion inflation
• Rotating Stars in Relativity
• A Global Model For Circumgalactic and Cluster-Core Precipitation
• Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA
• Raining on black holes and massive galaxies: the top-down multiphase condensation model
• Three-dimensional simulations of super-critical black hole accretion disks --- luminosities, photon trapping and variability
• Consequences of Strong Compression in Tidal Disruption Events
• Testing Primordial Black Holes as Dark Matter through LISA
• Low Luminosity Companions to White Dwarfs
• Dynamical evolution of black hole sub-systems in idealised star clusters
• Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
• Distant future of the Sun and Earth revisited
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• Near Infrared Spectroscopy of High Redshift Active Galactic Nuclei. I. A Metallicity-Accretion Rate Relationship
• Tidal Disruption Events Prefer Unusual Host Galaxies
• Modeling Dense Star Clusters in the Milky Way and Beyond with the $\text{CMC}$ Cluster Catalog
• Ultra-stripped Type Ic supernovae from close binary evolution
• Predicting the direction of the final spin from the coalescence of two black holes
• Simulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid Codes
• Limiting eccentricity of sub-parsec massive black hole binaries surrounded by self-gravitating gas discs
• Radiative and Momentum Based Mechanical AGN Feedback in a 3-Dimensional Galaxy Evolution Code
• The cosmic merger rate of neutron stars and black holes
• The Spin of the Supermassive Black Hole in NGC 3783
• The ELM Survey. I. A Complete Sample of Extremely Low Mass White Dwarfs
• A ~50,000 solar mass black hole in the nucleus of RGG 118
• Growth and activity of black holes in galaxy mergers with varying mass ratios
• Journey to the M_BH -sigma relation: the fate of low mass black holes in the Universe
• Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions
• Hangup Kicks: Still Larger Recoils by Partial Spin/Orbit Alignment of Black-Hole Binaries
• The Stellar Initial Mass Function of Ultra-Faint Dwarf Galaxies: Evidence for IMF Variations with Galactic Environment
• Black hole mass and spin coevolution by mergers
• The observed velocity distribution of young pulsars
• Dual Jets from Binary Black Holes
• Double neutron stars: merger rates revisited
• Radio Properties of Tidal Disruption Events
• Signatures of primordial black hole dark matter
• Exploring black hole superkicks
• Advanced burning stages and fate of 8-10 Mo stars
• On the alpha formalism for the common envelope interaction
• Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
• Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
• A wide star-black-hole binary system from radial-velocity measurements
• Dark Matter Spikes and Annihilation Radiation from the Galactic Center
• High-redshift galaxies, their active nuclei and central black holes
• The Spatial Distribution of Coalescing Neutron Star Binaries: Implications for Gamma-Ray Bursts
• Black holes and core expansion in massive star clusters
• The Pair-Instability Mass Gap for Black Holes
• Co-Evolution of Galactic Nuclei and Globular Cluster Systems
• Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform
• LISA verification binaries with updated distances from Gaia Data Release 2
• X-ray Polarization from Accreting Black Holes: II. The Thermal State
• Prelude to a double degenerate merger: the onset of mass transfer and its impact on gravitational waves and surface detonations
• Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey
• Collisions of white dwarfs as a new progenitor channel for type Ia supernovae
• Circumbinary MHD Accretion into Inspiraling Binary Black Holes
• Theory-Agnostic Constraints on Black-Hole Dipole Radiation with Multi-Band Gravitational-Wave Astrophysics
• Optical-Ultraviolet Tidal Disruption Events
• Intermediate-mass black holes in dwarf galaxies out to redshift $\sim$ 2.4 in the Chandra COSMOS Legacy Survey
• Gravitational-wave cosmology across 29 decades in frequency
• Black hole and neutron star mergers in galactic nuclei
• Rapid growth of seed black holes in the early universe by supra-exponential accretion
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes
• Gravitational Recoil From Accretion-Aligned Black-Hole Binaries
• Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
• On the Binding Energy Parameter $\lambda$ of Common Envelope Evolution
• Black hole mergers: can gas discs solve the `final parsec' problem?
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• Relativistic boost as the cause of periodicity in a massive black-hole binary candidate
• Simulations of star formation in a gaseous disc around sgr A* - a failed AGN
• Merging Binaries in the Galactic Center: The eccentric Kozai-Lidov mechanism with stellar evolution
• Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing
• Linking the spin evolution of massive black holes to galaxy kinematics
• The need for a second black hole at the Galactic center
• High-Density Effects in X-ray Reflection Models from Accretion Disks
• A dozen new galaxies caught in the act: Gas stripping and extended emission line regions in the Coma cluster
• Triangulation of gravitational wave sources with a network of detectors
• Imprints of Primordial Non-Gaussianity on Gravitational Wave Spectrum
• Time-Dependent Models for Dark Matter at the Galactic Center
• Properties of the Remnant Clockwise Disk of Young Stars in the Galactic Center
• A Giant Planet Candidate Transiting a White Dwarf
• Intermediate mass black holes in AGN disks II. Model predictions & observational constraints
• LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation
• High-spin binary black hole mergers
• Black Hole Mergers From Globular Clusters Observable by LISA I: Eccentric Sources Originating From Relativistic $N$-body Dynamics
• Fast coalescence of massive black hole binaries from mergers of galactic nuclei: implications for low-frequency gravitational-wave astrophysics
• Main-sequence stellar eruption model for V838 Mon
• Greatly enhanced merger rates of compact-object binaries in non-spherical nuclear star clusters
• X-rays across the galaxy population - II. The distribution of AGN accretion rates as a function of stellar mass and redshift
• Dynamics of triple black hole systems in hierarchically merging massive galaxies
• The binarity of the local white dwarf population
• Analysis of the Quiescent Low-Mass X-ray Binary Population in Galactic Globular Clusters
• A New Signature of Dark Matter Annihilations: Gamma-Rays from Intermediate-Mass Black Holes
• Low-mass black holes as the remnants of primordial black hole formation
• Deep Transfer Learning: A new deep learning glitch classification method for advanced LIGO
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• Off the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations
• Glitch Classification and Clustering for LIGO with Deep Transfer Learning
• Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
• Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters
• The LISA Gravitational Wave Foreground: A Study of Double White Dwarfs
• The gravitational wave signal from massive black hole binaries and its contribution to the LISA data stream
• Massive binary black holes in galactic nuclei and their path to coalescence
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• The Local Nanohertz Gravitational-Wave Landscape From Supermassive Black Hole Binaries
• Gravitational waves from cosmological compact binaries
• The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
• Remnant Masses, Spins and Recoils from the Merger of Generic Black-Hole Binaries
• The Discovery of Tidal Tails Around NGC 5466
• Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations
• Growth of structure seeded by primordial black holes
• Formation of Double Compact Objects
• The JWST Extragalactic Mock Catalog: Modeling galaxy populations from the UV through the near-IR over thirteen billion years of cosmic history
• Formation of black widows and redbacks -- two distinct populations of eclipsing binary millisecond pulsars
• An unusually brilliant transient in the galaxy Messier 85
• Low-frequency gravitational waves from supermassive black holes
• Evolution of binary black holes in self gravitating discs: dissecting the torques
• Black-Hole Spin and Galactic Morphology
• Survival of a brown dwarf after engulfment by a red giant star
• The Observational Signatures of Supermassive Black Hole Seeds
• Early Structure Formation in $\Lambda$PBH Cosmologies
• A planetesimal orbiting within the debris disc around a white dwarf star
• Capture of stellar--mass compact objects by massive black holes in galactic cusps
• The Evolution of Supermassive Population III Stars
• Use of gravitational waves to probe the formation channels of compact binaries
• Black hole evolution: III. Statistical properties of mass growth and spin evolution using large-scale hydrodynamical cosmological simulations
• Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals
• Initial mass function of intermediate mass black hole seeds
• Velocity Dispersions and X-Ray Temperatures of Galaxy Clusters
• The mass distribution of Galactic double neutron stars
• Feedback-regulated Super Massive Black Hole Seed Formation
• Massive main sequence stars evolving at the Eddington limit
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• The final-parsec problem in the collisionless limit
• Tides in rotating barotropic fluid bodies: the contribution of inertial waves and the role of internal structure
• Stellar Dynamics and Stellar Phenomena Near A Massive Black Hole
• Evolution of Giant Planets in Eccentric Disks
• Gravitational Wave and X-ray Signals from Stellar Disruption by a Massive Black Hole
• Evolution of the Dark Matter Distribution at the Galactic Center
• A new probe of dark matter properties: gravitational waves from an intermediate mass black hole embedded in a dark matter mini-spike
• Core depletion from coalescing supermassive black holes
• Distinguishing Between Formation Channels for Binary Black Holes with LISA
• A 12 minute Orbital Period Detached White Dwarf Eclipsing Binary
• eLISA eccentricity measurements as tracers of binary black hole formation
• Dual black holes in merger remnants. II: spin evolution and gravitational recoil
• Accretion of a giant planet onto a white dwarf
• Global Radiation Magneto-hydrodynamic Simulations of Sub-Eddington Accretion Disks around Supermassive Black Holes
• Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
• Linking Macro, Meso, and Micro Scales in Multiphase AGN Feeding and Feedback
• Orbital evolution of eccentric planets in radiative discs
• MOCCA Code for Star Cluster Simulations - II. Comparison with N-body Simulations
• Origin and growth of nuclear star clusters around massive black holes
• Gravitational-wave emission from compact Galactic binaries
• A Population of Bona Fide Intermediate Mass Black Holes Identified as Low Luminosity Active Galactic Nuclei
• Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems
• Observational Properties of Thermonuclear Supernovae
• Massive black hole binaries: dynamical evolution and observational signatures
• Gravitational collapse in f(R) theories
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• SMBH Formation via Gas Accretion in Nuclear Stellar Clusters
• Estimates of black-hole natal kick velocities from observations of low-mass X-ray binaries
• Ram pressure feeding super-massive black holes
• Reconstructing the massive black hole cosmic history through gravitational waves
• General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system
• Post Common Envelope Binaries from SDSS. I: 101 white dwarf main sequence binaries with multiple SDSS spectroscopy
• Post-Newtonian Evolution of Massive Black Hole Triplets in Galactic Nuclei: IV. Implications for LISA
• Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
• Population Synthesis of Binary Carbon-enhanced Metal-poor Stars
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation II
• Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach
• Galaxy Zoo: An independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS
• Cosmological constraints with deep learning from KiDS-450 weak lensing maps
• The evolution of active galactic nuclei and their spins
• Black Hole and Neutron Star Binary Mergers in Triple Systems: Merger Fraction and Spin-Orbit Misalignment
• POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations
• On the Rate of Neutron Star Binary Mergers from Globular Clusters
• The Evolution of the Globular Cluster System in a Triaxial Galaxy: Can a Galactic Nucleus Form by Globular Cluster Capture?
• Second-order self-force calculation of the gravitational binding energy in compact binaries
• Galactic binary science with the new LISA design
• Monte-Carlo simulations of black hole mergers in AGN disks: Low ${\chi }_{\mathrm{eff}}$ mergers and predictions for LIGO
• On the evolution of eccentric and inclined protoplanets embedded in protoplanetary disks
• Confusion Noise from LISA Capture Sources
• Constraints from Gravitational Recoil on the Growth of Supermassive Black Holes at High Redshift
• On the number density of "direct collapse" black hole seeds
• The Mass-Loss Induced Eccentric Kozai Mechanism: A New Channel for the Production of Close Compact Object-Stellar Binaries
• Formation of Millisecond Pulsars with Heavy White Dwarf Companions - Extreme Mass Transfer on Sub-Thermal Timescales
• Searching for Eccentricity: Signatures of Dynamical Formation in the First Gravitational-Wave Transient Catalogue of LIGO and Virgo
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• A top-heavy stellar initial mass function in starbursts as an explanation for the high mass-to-light ratios of ultra compact dwarf galaxies
• LISA Data Analysis using MCMC methods
• High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube
• The First Population II Stars Formed in Externally Enriched Mini-halos
• The effect of common-envelope evolution on the visible population of post-common-envelope binaries
• MOCCA code for star cluster simulations - I. Blue Stragglers, first results
• Multimessenger Signatures of Massive Black Holes in Dwarf Galaxies
• Hydrodynamic Torques in Circumbinary Accretion Disks
• The Triple Pulsar System PSR B1620-26 in M4
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• The ecology of star clusters and intermediate mass black holes in the Galactic bulge
• Scattering experiments meet N-body I: a practical recipe for the evolution of massive black hole binaries in stellar environments
• Formation and evolution of compact binaries in globular clusters: I.Binaries with white dwarfs
• The Mock LISA Data Challenges: from Challenge 3 to Challenge 4
• Tests of Bayesian Model Selection Techniques for Gravitational Wave Astronomy
• Recoiling Black Holes in Merging Galaxies: Relationship to AGN Lifetimes, Starbursts, and the M-sigma Relation
• Binary Black-Hole Mergers in Magnetized Disks: Simulations in Full General Relativity
• Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation
• A systematic search for massive black hole binaries in SDSS spectroscopic sample
• Binary black holes in young star clusters: the impact of metallicity
• Alternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1
• On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs
• The Distribution of Recoil Velocities from Merging Black Holes
• Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors
• Simulating the interstellar medium and stellar feedback on a moving mesh: Implementation and isolated galaxies
• High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants
• Black hole mergers from quadruples
• Binary black holes in the pair-instability mass gap
• The evolution of stellar triples: The most common evolutionary pathways
• Pairing of Supermassive Black Holes in unequal-mass galaxy mergers
• The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
• The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems
• Black Holes at the Centers of Nearby Dwarf Galaxies
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data II. Evolution of Clumpy Galaxies
• Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
• Black hole, neutron star and white dwarf merger rates in AGN disks
• Using transfer learning to detect galaxy mergers
• BSE versus StarTrack: implementations of new wind, remnant-formation, and natal-kick schemes in NBODY7 and their astrophysical consequences
• Fundamentals of the orbit and response for TianQin
• Learning Bayesian posteriors with neural networks for gravitational-wave inference
• Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
• Magnetospheres of Black Hole Systems in Force-Free Plasma
• Detecting a Stochastic Gravitational Wave Background in the presence of a Galactic Foreground and Instrument Noise
• Binary Encounters With Supermassive Black Holes: Zero-Eccentricity LISA Events
• Mass Transfer from Giant Donors
• Gravitational Recoil of Inspiralling Black-Hole Binaries to Second Post-Newtonian Order
• On Type Ia Supernovae From The Collisions of Two White Dwarfs
• Hydrodynamics of galaxy mergers with supermassive black holes: is there a last parsec problem ?
• Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries
• Circumbinary Accretion from Finite and Infinite Disks
• Multi-timescale analysis of phase transitions in precessing black-hole binaries
• Retention of Stellar-Mass Black Holes in Globular Clusters
• Optical Spectroscopy and Velocity Dispersions of Galaxy Clusters from the SPT-SZ Survey
• Formation of Double Neutron Star systems as implied by observations
• Gas-driven inspiral of binaries in thin accretion disks
• Stellar Evolution in AGN Disks
• Discovery of eight z ~ 6 quasars from Pan-STARRS1
• The late inspiral of supermassive black hole binaries with circumbinary gas discs in the LISA band
• From the first stars to the first black holes
• The Probability Distribution of Binary Pulsar Coalescence Rates. I. Double Neutron Star Systems in the Galactic Field
• The erratic dynamical life of black hole seeds in high-redshift galaxies
• Binary Black Hole Accretion During Inspiral and Merger
• A close-pair binary in a distant triple supermassive black-hole system
• Observational Signatures of Binary Supermassive Black Holes
• On the orientation and magnitude of the black hole spin in galactic nuclei
• Super-Eddington growth of the first black holes
• Deep radio imaging of 47 Tuc identifies the peculiar X-ray source X9 as a new black hole candidate
• MOCCA-SURVEY Database I: Galactic Globular Clusters Harbouring a Black Hole Subsystem
• Binaries migrating in a gaseous disk: Where are the Galactic center binaries?
• Stellar Dynamics of Extreme-Mass-Ratio Inspirals
• Accretion disks around binary black holes of unequal mass: GRMHD simulations near decoupling
• LISA double black holes: Dynamics in gaseous nuclear discs
• The Multi-Messenger Matrix: the Future of Neutron Star Merger Constraints on the Nuclear Equation of State
• Limits on primordial black holes from $\mu$ distortions in cosmic microwave background
• Further insight into gravitational recoil
• Binary black hole mergers: large kicks for generic spin orientations
• Chaotic cold accretion on to black holes in rotating atmospheres
• The Complete Evolution of a Neutron-Star Binary through a Common Envelope Phase Using 1D Hydrodynamic Simulations
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 $\le$ z $\le$ 7.0
• Probing the existence of ultralight bosons with a single gravitational-wave measurement
• Global Analysis of the Gravitational Wave Signal from Galactic Binaries
• Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor
• Dynamical evolution of intermediate mass black holes and their observable signatures in the nearby Universe
• Formation of Massive Black Holes in Galactic Nuclei: Runaway Tidal Encounters
• Constraints on the astrophysical environment of binaries with gravitational-wave observations
• Transient resonances in the inspirals of point particles into black holes
• Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements
• Recoiling black holes: prospects for detection and implications of spin alignment
• Unveiling the first black holes with JWST: multi-wavelength spectral predictions
• Characterizing the Galactic Gravitational Wave Background with LISA
• The Formation and Gravitational-Wave Detection of Massive Stellar Black-Hole Binaries
• Gravitational self-force on generic bound geodesics in Kerr spacetime
• A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
• Characterization of the stochastic signal originating from compact binaries populations as measured by LISA
• The Role of Helium Stars in the Formation of Double Neutron Stars
• The Parkes Pulsar Timing Array Project: Second data release
• On the Formation and Evolution of Common Envelope Systems
• High redshift radio galaxies and divergence from the CMB dipole
• Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO
• Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
• Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes
• Wandering Black Holes in Bright Disk Galaxy Halos
• Effective potentials and morphological transitions for binary black-hole spin precession
• Quantifying the impact of the Large Magellanic Cloud on the structure of the Milky Way's dark matter halo using Basis Function Expansions
• Growing massive black holes through super-critical accretion of stellar-mass seeds
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• An astrometric search method for individually resolvable gravitational wave sources with Gaia
• Simple recipes for compact remnant masses and natal kicks
• The (black hole)-bulge mass scaling relation at low masses
• Surrounded by Spiders! New Black Widows and Redbacks in the Galactic Field
• Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
• On the Binding Energy Parameter of Common Envelope Evolution. Dependency on the Definition of the Stellar Core Boundary during Spiral-in
• Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms
• The influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals
• Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background
• Dynamical Friction around Supermassive Black Holes
• On the possibility of a helium white dwarf donor in the presumed ultracompact binary 2S 0918-549
• Gravitational Waves and Intermediate-mass Black Hole Retention in Globular Clusters
• Gaia DR2 Distances and Peculiar Velocities for Galactic Black Hole Transients
• A population of intermediate-mass black holes in dwarf starburst galaxies up to redshift=1.5
• Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution
• The chemical composition of donors in AM CVn stars and ultra-compact X-ray binaries: observational tests of their formation
• Neutron Star Kicks in Isolated and Binary Pulsars: Observational Constraints and Implications for Kick Mechanisms
• A progenitor binary and an ejected mass donor remnant of faint type Ia supernovae
• Growing Massive Black Hole Pairs in Minor Mergers of Disk Galaxies
• A systematic search of Zwicky Transient Facility data for ultracompact binary LISA-detectable gravitational-wave sources
• Accretion in common envelope evolution
• Gravitational recoil: signatures on the massive black hole population
• Measuring the star formation rate with gravitational waves from binary black holes
• Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{\ast ,sph}$ and $M_{BH}$-$M_{\ast ,gal}$
• Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays
• A transition in circumbinary accretion discs at a binary mass ratio of 1:25
• Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes
• Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549
• Population synthesis of triple systems in the context of mergers of carbon-oxygen white dwarfs
• The formation of galaxy stellar cores by the hierarchical merging of supermassive black holes
• How to observe a non-Kerr spacetime
• Every interacting double white dwarf binary may merge
• The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
• Binary Black Hole Mergers in Gaseous Environments: "Binary Bondi" and "Binary Bondi-Hoyle-Lyttleton" Accretion
• Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters
• AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
• Thermal disc emission from a rotating black hole: X-ray polarization signatures
• Nuclear-dominated accretion and subluminous supernovae from the merger of a white dwarf with a neutron star or black hole
• Dynamical friction and the evolution of Supermassive Black hole Binaries: the final hundred-parsec problem
• Rapid Orbital Decay in the 12.75-minute WD+WD Binary J0651+2844
• Ultracompact X-Ray Binaries with Neon-Rich Degenerate Donors
• Doppler-imaging of the planetary debris disc at the white dwarf SDSS J122859.93+104032.9
• An Overabundance of Black Hole X-Ray Binaries in the Galactic Center from Tidal Captures
• Mass transfer from a giant star to a main sequence companion and its contribution to long-orbital-period blue stragglers
• Massive black holes lurking in Milky Way satellites
• Common Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes
• Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
• Hidden AGN in dwarf galaxies revealed by MaNGA: light echoes, off-nuclear wanderers, and a new broad-line AGN
• The First Billion Years project: birthplaces of direct collapse black holes
• Recoiling black holes: electromagnetic signatures, candidates, and astrophysical implications
• The ELM Survey. VIII. 98 Double White Dwarf Binaries
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Galaxy Zoo: CANDELS Barred Disks and Bar Fractions
• Formation pathway of Population III coalescing binary black holes through stable mass transfer
• The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries
• Direct collapse black hole formation from synchronized pairs of atomic cooling halos
• Evolution of Massive Black Hole Binaries
• Inferring the Inclination of a Black Hole Accretion Disk from Observations of its Polarized Continuum Radiation
• Repeated mergers and ejection of black holes within nuclear star clusters
• The formation of low-mass helium white dwarfs orbiting pulsars: Evolution of low-mass X-ray binaries below the bifurcation period
• Massive Black Hole Binaries from Collisional Runaways
• The influence of the distribution of cosmic star formation at different metallicities on the properties of merging double compact objects
• Mergers of Unequal Mass Galaxies: Supermassive Black Hole Binary Evolution and Structure of Merger Remnants
• Long-Term Evolution of Massive Black Hole Binaries. II. Binary Evolution in Low-Density Galaxies
• Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
• Effects of gravitational-wave recoil on the dynamics and growth of supermassive black holes
• The power spectrum on small scales: Robust constraints and comparing PBH methodologies
• Optimizing orbits for TianQin
• The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies
• Recombination energy in double white dwarf formation
• Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
• Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
• Revising natal kick prescriptions in population synthesis simulations
• Constraining sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. I. The General Quasar Population
• Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes
• Thin accretion disk signatures in dynamical Chern-Simons modified gravity
• Detection Rate Estimates of Gravity-waves Emitted During Parabolic Encounters of Stellar Black Holes in Globular Clusters
• Core Formation in Galactic Nuclei Due to Recoiling Black Holes
• The LISA verification binaries
• MOCCA-SURVEY Database I. Unravelling black hole subsystems in globular clusters
• The Growth of Black Holes from Population III Remnants in the Renaissance Simulations
• Stellar-mass black holes in young massive and open stellar clusters IV: updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data
• Advection Dominated Accretion Flows in the Kerr Metric: II. Steady State Global Solutions
• The ALMA Spectroscopic Survey in the HUDF: Multi-band constraints on line luminosity functions and the cosmic density of molecular gas
• Stochastic Gravitational-Wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
• Intermediate Mass Black Hole Formation in compact Young Massive Star Clusters
• Black hole masses of tidal disruption event host galaxies II
• Tidally induced bars in Illustris galaxies
• The spatial clustering of X-ray selected AGN and galaxies in the Chandra Deep Field South and North
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• Post-Newtonian Dynamics in Dense Star Clusters: Binary Black Holes in the LISA Band
• Electromagnetic Emission from Supermassive Binary Black Holes Approaching Merger
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• Evolution of Low-Mass Helium Stars in Semidetached Binaries
• Three-Dimensional Simulations of Tidally Disrupted Solar-Type Stars and the Observational Signatures of Shock Breakout
• The ELM Survey. IV. 24 White Dwarf Merger Systems
• Aligning Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disk
• Predicting the binary black hole population of the Milky Way with cosmological simulations
• Formation of the Galactic Millisecond Pulsar Triple System PSR J0337+1715 - a Neutron Star with Two Orbiting White Dwarfs
• Close Binary White Dwarf Systems: Numerous New Detections and Their Interpretation
• X-ray Detected Active Galactic Nuclei in Dwarf Galaxies at $0<z<1$
• Multiband gravitational-wave event rates and stellar physics
• Population synthesis of black hole binary mergers from star clusters
• An observable signature of a background deviating from Kerr
• The X-ray Halo Scaling Relations of Supermassive Black Holes
• Binaries discovered by the SPY project. IV. Five single-lined DA double white dwarfs
• Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{sph}}$
• Galaxy bulges and their massive black holes: a review
• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• Tidal resonance in extreme mass-ratio inspirals
• AI-assisted super-resolution cosmological simulations
• Multi-band gravitational-wave astronomy: parameter estimation and tests of general relativity with space and ground-based detectors
• Intermediate-mass Black Holes from High Massive-star Binary Fractions in Young Star Clusters
• Dynamical evolution of the young stars in the Galactic center: N-body simulations of the S-stars
• General Relativistic Simulations of Magnetized Plasmas around Merging Supermassive Black Holes
• Dancing to ChaNGa: A Self-Consistent Prediction For Close SMBH Pair Formation Timescales Following Galaxy Mergers
• Detecting triple systems with gravitational wave observations
• Prompt Shocks in the Gas Disk Around a Recoiling Supermassive Black Hole Binary
• Supermassive Black Hole Binary Candidates from the Pan-STARRS1 Medium Deep Survey
• Optical Thermonuclear Transients From Tidal Compression of White Dwarfs as Tracers of the Low End of the Massive Black Hole Mass Function
• Fingerprints of binary black hole formation channels encoded in the mass and spin of merger remnants
• Simulating merging binary black holes with nearly extremal spins
• Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal
• Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
• Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back)
• Optical spectroscopy of (candidate) ultra-compact X-ray binaries: constraints on the composition of the donor stars
• Black Hole Mergers From Globular Clusters Observable by LISA II: Resolved Eccentric Sources and the Gravitational Wave Background
• The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
• PopCORN: Hunting down the differences between binary population synthesis codes
• Mergers and ejections of black holes in globular clusters
• The Infrared Afterglow of Supermassive Black Hole Mergers
• How initial size governs core collapse in globular clusters
• Swift spectra of AT2018cow: A White Dwarf Tidal Disruption Event?
• Spectroscopic Evidence for a 5.4-Minute Orbital Period in HM Cancri
• The distribution of old stars around the Milky Way's central black hole I: Star counts
• Mass transfer in white dwarf-neutron star binaries
• The Globular Cluster Migratory Origin of Nuclear Star Clusters
• A lower fragmentation mass scale in high redshift galaxies and its implications on giant clumps: a systematic numerical study
• Direct formation of supermassive black holes in metal-enriched gas at the heart of high-redshift galaxy mergers
• Neutron Star Kicks and their Relationship to Supernovae Ejecta Mass
• Discovery of a relationship between spiral arm morphology and supermassive black hole mass in disk galaxies
• On the Accretion-Fed Growth of Neutron Stars During Common Envelope
• Magnetic Interactions in Coalescing Neutron Star Binaries
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Perturbations of Intermediate-mass Black Holes on Stellar Orbits in the Galactic Center
• Steady state relativistic stellar dynamics around a massive black hole
• Formation of massive seed black holes via collisions and accretion
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• The 6dF Galaxy Survey: Bulk Flows on $50-70h^{-1}$ Mpc scales
• A limit on eccentricity growth from global 3-D simulations of disc-planet interactions
• Detection of Supermassive Black Holes in Two Virgo Ultracompact Dwarf Galaxies
• Image-based deep learning for classification of noise transients in gravitational wave detectors
• The physical properties of AM CVn stars: new insights from Gaia DR2
• Runaway collisions in young star clusters. I. Methods and tests
• Constraints on Primordial Black Holes: the Importance of Accretion
• The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9
• Periodic self-lensing from accreting massive black hole binaries
• Are we there yet? Time to detection of nanohertz gravitational waves based on pulsar-timing array limits
• The effect of stellar-mass black holes on the structural evolution of massive star clusters
• Constraining the Orbit of Supermassive Black Hole Binary 0402+379
• Be X-ray binaries in the SMC as indicators of mass transfer efficiency
• The Fate of Binaries in the Galactic Center: The Mundane and the Exotic
• Search for Supermassive Black Hole Binaries in the Sloan Digital Sky Survey Spectroscopic Sample
• Collisionless loss-cone refilling: there is no final parsec problem
• Gravitational waves from the Papaloizou-Pringle instability in black hole-torus systems
• The spin-flip phenomenon in supermassive black hole binary mergers
• PRECESSION: Dynamics of spinning black-hole binaries with python
• The equilibrium tide in stars and giant planets: I - the coplanar case
• Interaction of massive black hole binaries with their stellar environment: III. Scattering of bound stars
• Multiple stellar-mass black holes in globular clusters: theoretical confirmation
• Revealing black holes with Gaia
• Radial velocity measurements of white dwarfs
• Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations
• Quasi-Periodic Behavior of Mini-Disks in Binary Black Holes Approaching Merger
• The timescale of low-mass proto-helium white dwarf evolution
• On the Formation of Helium Double Degenerate Stars and Pre-Cataclysmic Variables
• HST/FGS Parallaxes of AM CVn Stars and Astrophysical Consequences
• Massive Black Hole binaries in gas-rich galaxy mergers; multiple regimes of orbital decay and interplay with gas inflows
• Evolution of Galactic Nuclei with 10 $M_{\odot }$ Black Holes
• Black hole mergers: the first light
• Common envelope events with low-mass giants: understanding the energy budget
• LISA data analysis: Source identification and subtraction
• Constraining Sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. II. The Population with Kinematically Offset Broad Balmer Emission Lines
• Supermassive Star Formation via Super Competitive Accretion in Slightly Metal-enriched Clouds
• On the distribution of stellar remnants around massive black holes: slow mass segregation, star cluster inspirals and correlated orbits
• Detectability of Intermediate-Mass Black Holes in Multiband Gravitational Wave Astronomy
• Gauss's method for secular dynamics, softened
• Precessional dynamics of black hole triples: binary mergers with near-zero effective spin
• Collisions in Primordial Star Clusters: Formation Pathway for intermediate mass black holes
• On the detectability of dual jets from binary black holes
• PBH dark matter from axion inflation
• The ESO supernovae type Ia progenitor survey (SPY)
• Black Hole Mergers from Hierarchical Triples in Dense Star Clusters
• Nonlinear gravitational self-force: second-order equation of motion
• A new channel to form IMBHs throughout cosmic time
• Efficiency of Super-Eddington Magnetically-Arrested Accretion
• Understanding the evolution of close binary systems with radio pulsars
• Swift coalescence of supermassive black holes in cosmological mergers of massive galaxies
• The impact of realistic models of mass segregation on the event rate of extreme-mass ratio inspirals and cusp re-growth
• Triplets of supermassive black holes: Astrophysics, Gravitational Waves and Detection
• Understanding possible electromagnetic counterparts to loud gravitational wave events: Binary black hole effects on electromagnetic fields
• Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae
• Binary black holes' effects on electromagnetic fields
• Black hole-neutron star mergers from triples
• V407 Vul: a direct impact accretor
• The formation and evolution of bars in low surface brightness galaxies with cold dark matter halos
• Detectable environmental effects in GW190521-like black-hole binaries with LISA
• On the coexistence of stellar-mass and intermediate-mass black holes in globular clusters
• Are stellar-mass black-hole binaries too quiet for LISA?
• Wandering Supermassive Black Holes in Milky Way Mass Halos
• The distribution of stars around the Milky Way's black hole III: Comparison with simulations
• The evolution of ultracompact X-ray binaries
• Relativistic Suppression of Black Hole Recoils
• Star Captures by Quasar Accretion Disks: A Possible Explanation of the M-sigma Relation
• Depleted cores, multi-component fits, and structural parameter relations for luminous early-type galaxies
• Shining in the Dark: the Spectral Evolution of the First Black Holes
• A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes - III. Radial Velocity Variations
• An alternative method to study star cluster disruption
• When and where did GW150914 form?
• Secular Stellar Dynamics near a Massive Black Hole
• A New Estimation of Mass Accumulation Efficiency in Helium Shell Flashes toward Type Ia Supernova Explosions
• Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• Mini-dark halos with intermediate mass black holes
• Evolution of Galactic Nuclei. I. orbital evolution of IMBH
• Post-Newtonian evolution of massive black hole triplets in galactic nuclei -- II. Survey of the parameter space
• Vacuum Electromagnetic Counterparts of Binary Black-Hole Mergers
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• An electrically powered binary star?
• Atypical Thermonuclear Supernovae from Tidally Crushed White Dwarfs
• Black Hole Mass Scaling Relations for Spiral Galaxies. II. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{tot}}$ and $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{disk}}$
• Massive black hole pairs in clumpy, self-gravitating circumnuclear disks: stochastic orbital decay
• Resonant Tidal Excitation of Oscillation Modes in Merging Binary Neutron Stars: Inertial-Gravity Modes
• Brownian Motion of a Massive Binary
• Episodic mass ejections from common-envelope objects
• Galaxy Rotation and Rapid Supermassive Black Hole Binary Coalescence
• Disentangling Coalescing Neutron Star-White Dwarf Binaries for LISA
• Probing Massive Black Hole Binary Populations with LISA
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Dynamics of black hole - neutron star binaries in young star clusters
• Spin-Orbit Misalignment of Merging Black-Hole Binaries with Tertiary Companions
• A numerical study of vector resonant relaxation
• Iron Opacity Bump Changes the Stability and Structure of Accretion Disks in Active Galactic Nuclei
• LISA sources in Milky Way globular clusters
• The gravitational wave signal from diverse populations of double white dwarf binaries in the Galaxy
• Exploring intermediate and massive black-hole binaries with the Einstein Telescope
• Supermassive black holes from primordial black hole seeds
• Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
• Suppression of the accretion rate in thin discs around binary black holes
• The rate of WD-WD head-on collisions in isolated triples is too low to explain standard type Ia supernovae
• Research Update on Extreme-Mass-Ratio Inspirals
• The MEGaN project II. Gravitational waves from intermediate mass- and binary black holes around a supermassive black hole
• Gravitational waves from the electroweak phase transition
• S62 and S4711: Indications of a population of faint fast moving stars inside the S2 orbit -- S4711 on a 7.6 year orbit around Sgr~A*
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Powerful flares from recoiling black holes in quasars
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• The Effect of Massive Perturbers on Extreme Mass-Ratio Inspiral Waveforms
• On the formation of the first quasars
• Evidence for periodicity in 43 year-long monitoring of NGC 5548
• Formation of galactic nuclei with multiple supermassive black holes at high redshifts
• Gravitational wave background from extreme mass ratio inspirals
• Extending Common Envelope Simulations from Roche Lobe Overflow to the Nebular Phase
• Euclid preparation: V. Predicted yield of redshift 7<z<9 quasars from the wide survey
• Intermediate mass black holes from stellar mergers in young star clusters
• Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
• On the Formation of Double White Dwarfs through Stable Mass Transfer and a Common Envelope
• Constraining Sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. III. Candidates from Continued Radial Velocity Tests
• Nonlinear Gravitational Recoil from the Mergers of Precessing Black-Hole Binaries
• The quest for companions to post-common envelope binaries: III. A reexamination of HW Virginis
• Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc
• The origin and fate of short-period low-mass black-hole binaries
• A selection effect boosting the contribution from rapidly spinning black holes to the Cosmic X-ray Background
• Gravitational-Wave Emission from Binary Black Holes Formed in Open Clusters
• Companion-launched jets and their effect on the dynamics of common envelope interaction simulations
• Supermassive black holes formed by direct collapse of inflationary perturbations
• Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order
• A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
• Ultracompact AM CVn Binaries from the Sloan Digital Sky Survey: Three Candidates Plus the First Confirmed Eclipsing System
• Nuclear Dominated Accretion Flows in Two Dimensions. I. Torus Evolution with Parametric Microphysics
• On the formation of neutron stars via accretion-induced collapse in binaries
• Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background
• Accreting Double white dwarf binaries: Implications for LISA
• Growth of eccentric modes in disc-planet interactions
• Dynamical Tides in Compact White Dwarf Binaries: Tidal Synchronization and Dissipation
• Analytical expressions for the envelope binding energy of giants as a function of basic stellar parameters
• Black Hole Formation in the Lower Mass Gap through Mergers and Accretion in AGN Disks
• Detecting hierarchical stellar systems with LISA
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• Final spins from the merger of precessing binary black holes
• The Effect of Star--Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events
• Extreme mass ratio inspirals with spinning secondary: a detailed study of equatorial circular motion
• Massive black hole binary eccentricity in rotating stellar systems
• Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems
• Evolution of Close White Dwarf Binaries
• Fossil Gas and the Electromagnetic Precursor of Supermassive Binary Black Hole Mergers
• Hunting Black Holes with Gaia
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks
• Revealing Hidden Substructures in the $M_{BH}$-$\sigma$ Diagram, and Refining the Bend in the $L$-$\sigma$ Relation
• Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes
• Detecting Intermediate-Mass Ratio Inspirals From The Ground And Space
• A practical, covariant puncture for second-order self-force calculations
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Numerical Relativity of Compact Binaries in the 21st Century
• Detecting Double Neutron Stars with LISA
• Central Stellar Mass Deficits in the Bulges of Local Lenticular Galaxies, and the Connection with Compact z ~ 1.5 Galaxies
• Star Formation in Accretion Disks and SMBH Growth
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• The peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA
• The shortest period sdB plus white dwarf binary CD-30 11223 (GALEX J1411-3053)
• The First Tidally Disrupted Ultra-Faint Dwarf Galaxy? - Spectroscopic Analysis of the Tucana III Stream
• Alignment of supermassive black hole binary orbits and spins
• The population of AM CVn stars from the Sloan Digital Sky Survey
• The Spitzer mid-infrared AGN survey. II-the demographics and cosmic evolution of the AGN population
• Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges
• Henize 2-10: the ongoing formation of a nuclear star cluster around a massive black hole
• Conditions for Optimal Growth of Black Hole Seeds
• A search for the hidden population of AM CVn binaries in the Sloan Digital Sky Survey
• Estimates of Black Hole Spin Properties of 55 Sources
• The formation of extremely diffuse galaxy cores by merging supermassive black holes
• The numerical relativity breakthrough for binary black holes
• CMB constraints on primordial black hole dark matter
• An enhanced rate of tidal disruptions in the centrally overdense E+A galaxy NGC 3156
• Disk Evolution and Bar Triggering Driven by Interactions with Dark Matter Substructure
• Gravitational radiation from a torus around a black hole
• The High Time Resolution Universe Pulsar Survey VIII: The Galactic millisecond pulsar population
• A fully parallel, high precision, N-body code running on hybrid computing platforms
• Constraining scalar fields with stellar kinematics and collisional dark matter
• Populating the low-mass end of the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• A new Fokker-Planck approach for relaxation-driven evolution of galactic nuclei
• Relativistic Motion of Spinning Particles in a Gravitational Field
• eROSITA on SRG
• The electromagnetic chirp of a compact binary black hole: a phase template for the gravitational wave inspiral
• Black Hole Disks in Galactic Nuclei
• H_2 Suppression with Shocking Inflows: Testing a Pathway for Supermassive Black Hole Formation
• Intermediate-mass black holes in colliding clusters: Implications for lower-frequency gravitational-wave astronomy
• Star-disc interaction in galactic nuclei: orbits and rates of accreted stars
• Most Double Degenerate Low Mass White Dwarf Binaries Merge
• On the formation of GW190814
• Magnetic Field Amplification During the Common Envelope Phase
• Populations of double white dwarfs in Milky Way satellites and their detectability with LISA
• The efficiency of resonant relaxation around a massive black hole
• The Close Stellar Companions to Intermediate Mass Black Holes
• Supermassive star formation via episodic accretion: protostellar disc instability and radiative feedback efficiency
• Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO
• Accuracy of the Post-Newtonian Approximation: Optimal Asymptotic Expansion for Quasi-Circular, Extreme-Mass Ratio Inspirals
• Gravitational waves from supermassive stars collapsing to a supermassive black hole
• Galactic nuclei evolution with spinning black holes: method and implementation
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• Quasi-Periodicity of Supermassive Binary Black Hole Accretion Approaching Merger
• Hydrodynamics of Rotating Stars and Close Binary Interactions: Compressible Ellipsoid Models
• Comparison of Gravitational Wave Detector Network Sky Localization Approximations
• Dynamics of compact objects clusters: A post-Newtonian study
• The first ultracompact Roche lobe-filling hot subdwarf binary
• Long-term evolution of compact binaries with irradiation feedback
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• The M - σrelation in different environments
• White dwarf pollution by planets in stellar binaries
• Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
• Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently
• The HU Aqr planetary system hypothesis revisited
• Kinematics of the ultra-compact helium accretor AM Canum Venaticorum
• Black hole feeding and feedback: the physics inside the "subgrid"
• Preserving Kerr symmetries in deformed spacetimes
• Off-nuclear AGN as a signature of recoiling massive black holes
• An ultracompact X-ray binary in the globular cluster M15 (NGC7078)
• Secular dynamics in hierarchical three-body systems with mass loss and mass transfer
• Constraints On The Dynamical Environments Of Supermassive Black-hole Binaries Using Pulsar-timing Arrays
• The Stability of Double White Dwarf Binaries Undergoing Direct Impact Accretion
• Mass-redshift Degeneracy for Gravitational-wave Sources in the Vicinity of a Supermassive Black Hole
• Tidal disruptions of main sequence stars -- II. Simulation methodology and stellar mass dependence of the character of full tidal disruptions
• A hidden friend for the galactic center black hole, Sgr A*
• Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
• Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
• Importance of transient resonances in extreme-mass-ratio inspirals
• Stellar Black Hole Binary Mergers in Open Clusters
• HST/WFPC2 imaging of the circumnuclear structure of LLAGNs. I Data and nuclear morphology
• Luminous Red Novae: population models and future prospects
• Detecting Supermassive Black Hole-Induced Binary Eccentricity Oscillations with LISA
• A New Type of Extreme-mass-ratio Inspirals Produced by Tidal Capture of Binary Black Holes
• Monte Carlo cluster simulations to determine the rate of compact star inspiraling to a central galactic black hole
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• Galactic Ultracompact X-ray Binaries: Disk Stability and Evolution
• Bayesian modeling of source confusion in LISA data
• Detecting Black Hole Binaries by Gaia
• Gravitational waves with dark matter minispikes: the combined effect
• Can We Trust Models for Adiabatic Mass Loss?
• Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
• Extracting the Gravitational Recoil from Black Hole Merger Signals
• The Dynamical Significance of Triple Star Systems in Star Clusters
• Common-envelope evolution with an asymptotic giant branch star
• Nuclear coups: dynamics of black holes in galaxy mergers
• Direct N-body simulation of the Galactic centre
• Cyg X-3: a Galactic double black hole or black hole-neutron star progenitor
• Distances to Galactic X-ray Binaries with Gaia DR2
• The Delay Time Distribution of Tidal Disruption Flares
• Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• Making a supermassive star by stellar bombardment
• Report on the second Mock LISA Data Challenge
• An Upper Limit on the Mass of a Primordial Star due to the Formation of an HII Region: The Effect of Ionizing Radiation Force
• Reaching the boundary between stellar kinematic groups and very wide binaries. The Washington Double Stars with the widest angular separations
• Mass without radiation: heavily obscured AGN, the X-ray Background and the Black Hole Mass Density
• X-MRIs: Extremely Large Mass-Ratio Inspirals
• Black hole kicks as new gravitational wave observables
• Merger rate density of binary black holes formed in open clusters
• Binary radial velocity measurements with space-based gravitational-wave detectors
• Gravitational waves from bodies orbiting the Galactic Center black hole and their detectability by LISA
• A-type Stars, the Destroyers of Worlds: The lives and deaths of Jupiters in evolving stellar binaries
• Supermassive black hole pairs in clumpy galaxies at high redshift: delayed binary formation and concurrent mass growth
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Detectability of ultra-compact X-ray binaries as LISA sources
• Evolution of inclined planets in three-dimensional radiative discs
• Characterizing accreting double white dwarf binaries with the Laser Interferometer Space Antenna and Gaia
• Gravitational recoils of supermassive black holes in hydrodynamical simulations of gas rich galaxies
• Black hole mergers in compact star clusters and massive black hole formation beyond the mass-gap
• Measuring the eccentricity of GW170817 and GW190425
• Black-hole kicks from numerical-relativity surrogate models
• Foreground cleaning and template-free stochastic background extraction for LISA
• Slowly, slowly in the wind: 3D hydrodynamical simulations of wind mass transfer and angular-momentum loss in AGB binary systems
• Tracking black hole kicks from gravitational wave observations
• Common-Envelope Episodes that lead to Double Neutron Star formation
• Kinetic and radiative power from optically thin accretion flows
• The triple degenerate star WD1704+481
• The astrophysical science case for a decihertz gravitational-wave detector
• Modelling the formation of double white dwarfs
• The role of the supermassive black hole spin in the estimation of the EMRI event rate
• Seeding Black Holes in Cosmological Simulations
• External versus internal triggers of bar formation in cosmological zoom-in simulations
• Pulsar Spin--Velocity Alignment: Further Results and Discussion
• Probing General Relativity With Mergers of Supermassive and Intermediate-Mass Black Holes
• Dissecting the turbulent weather driven by mechanical AGN feedback
• Using electromagnetic observations to aid gravitational-wave parameter estimation of compact binaries observed with LISA
• Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH
• Simulations of common envelope evolution in triple systems: Circumstellar case
• Massive perturbers and the efficient merger of binary massive black holes
• Candidate Periodically Variable Quasars from the Dark Energy Survey and the Sloan Digital Sky Survey
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• Monte Carlo simulations of post-common-envelope white dwarf + main sequence binaries: The effects of including recombination energy
• Further Evidence for a Supermassive Black Hole Mass - Pitch Angle Relation
• Considerations on the Role of Fall-Back Discs in the Final Stages of the Common Envelope Binary Interaction
• Spin alignment and differential accretion in merging black hole binaries
• Black Hole Binaries in Galactic Nuclei and Gravitational Wave Sources
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• Gone with the wind: the impact of wind mass transfer on the orbital evolution of AGB binary systems
• Prompt Electromagnetic Transients from Binary Black Hole Mergers
• Chandra High resolution Observations of CID-42, a candidate recoiling SMBH
• Accreting black hole binaries in globular clusters
• Migration of massive black hole binaries in self--gravitating accretion discs: Retrograde versus prograde
• Gravitational wave bursts from the Galactic massive black hole
• Astrophysical Model Selection in Gravitational Wave Astronomy
• Recoiling Supermassive Black Holes: a search in the Nearby Universe
• The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay between Radiative Cooling, Star Formation, and Feedback Processes
• The Formation of Stellar Black Holes
• SDSS J0926+3624: The shortest period eclipsing binary star
• A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes - II. Continued Spectroscopic Monitoring and Optical Flux Variability
• Very Broad [O III]4959,5007 Emission from the NGC 4472 Globular Cluster RZ2109 and Implications for the Mass of Its Black Hole X-ray Source
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Accurate Identification of Galaxy Mergers with Imaging
• An 8.8 minute orbital period eclipsing detached double white dwarf binary
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• Orbits Around Black Holes in Triaxial Nuclei
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Planet formation from the ejecta of common envelopes
• The Evolution of Binaries in a Gaseous Medium: Three-Dimensional Simulations of Binary Bondi-Hoyle-Lyttleton Accretion
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Eccentric double white dwarfs as LISA sources in globular clusters
• An algorithm for detection of extreme mass ratio inspirals in LISA data
• Pre-merger electromagnetic counterparts of binary compact stars
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• The tidal remnant of an unusually metal-poor globular cluster
• Exploring SMBH Assembly with Semi-analytic Modelling
• The birth of a supermassive black hole binary
• Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
• The nature of massive black hole binary candidates: I. Spectral properties and evolution
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Ripple effects & oscillations in the broad FeKa line as a probe of massive black hole mergers
• The White Dwarf -- White Dwarf galactic background in the LISA data
• Retaining Black Holes with Very Large Recoil Velocities
• Testing the relativistic Doppler boost hypothesis for supermassive black hole binary candidates
• Stirred and shaken: dynamical behavior of boson stars and dark matter cores
• MOCCA Survey Database I: Dissolution of tidally filling star clusters harbouring BH subsystems
• Where are the double-degenerate progenitors of type Ia supernovae?
• Effects of Intermediate Mass Black Holes on Nuclear Star Clusters
• Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window
• Magnetorotational collapse of very massive stars to black holes in full general relativity
• The Early Growth of the First Black Holes
• Spikey: Self-Lensing Flares from Eccentric SMBH Binaries
• A General Formula for Black Hole Gravitational Wave Kicks
• Relativity and the evolution of the Galactic center S-star orbits
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Gas depletion in primordial globular clusters due to accretion onto stellar-mass black holes
• Hydrodynamical Response of a Circumbinary Gas Disk to Black Hole Recoil and Mass Loss
• The mass ratio distribution of short period double degenerate stars
• Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
• Tidal disruption of dwarf spheroidal galaxies: the strange case of Crater II
• Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• The spin period - eccentricity relation of double neutron stars: evidence for weak supernova kicks?
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Tidal Interactions in Merging White Dwarf Binaries
• Resolving massive black hole binaries evolution via adaptive particle-splitting
• Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA "Verification Binaries"
• Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA
• Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity
• Opacity Driven Convection and Variability in Accretion Disks around Supermassive Black Holes
• Investigating spinning test particles: spin supplementary conditions and the Hamiltonian formalism
• Searching for Binary Supermassive Black Holes via Variable Broad Emission Line Shifts: Low Binary Fraction
• MOCCA-SURVEY Database I: Assessing GW kick retention fractions for BH-BH mergers in globular clusters
• An upper limit to the velocity dispersion of relaxed stellar systems without massive black holes
• Dark matter: an efficient catalyst for intermediate-mass-ratio-inspiral events
• Relativistic three-body effects in hierarchical triples
• Stability criteria for hierarchical triple systems
• Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects
• Effects of Wandering on the Coalescence of Black Hole Binaries in Galactic Centers
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• Precision X-ray Timing of RX J0806.3+1527 with CHANDRA: Evidence for Gravitational Radiation from an Ultracompact Binary
• General relativistic spin-orbit and spin-spin effects on the motion of rotating particles in an external gravitational field
• Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA
• Clumpy galaxies seen in H-alpha: inflated observed clump properties due to limited spatial resolution and sensitivity
• The puzzling case of the radio-loud QSO 3C 186: a gravitational wave recoiling black hole in a young radio source?
• A New Gravitational Wave Verification Source
• The effect of binding energy and resolution in simulations of the common envelope binary interaction
• Millimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way
• Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
• Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA and the next generation of gravitational wave detectors
• Effects of post-Newtonian Spin Alignment on the Distribution of Black-Hole Recoils
• Description of the Scenario Machine
• Formation of LISA Black Hole Binaries in Merging Dwarf Galaxies: the Imprint of Dark Matter
• Common Envelope Evolution on a Moving Mesh
• Type Ia Supernova Sub-classes and Progenitor Origin
• Star-disc interaction in galactic nuclei: formation of a central stellar disc
• Separating Accretion and Mergers in the Cosmic Growth of Black Holes with X-ray and Gravitational Wave Observations
• r-process enrichment of ultra-faint dwarf galaxies by fast merging double neutron stars
• The thermal equilibrium mass loss model and its applications in binary evolution
• A new class of Roche lobe-filling hot subdwarf binaries
• Multi-band gravitational wave tests of general relativity
• Reduced magnetic braking and the magnetic capture model for the formation of ultra-compact binaries
• Observing the Galaxy's massive black hole with gravitational wave bursts
• Detectability of double white dwarfs in the Local Group with LISA
• Calculation of radiation reaction effect on orbital parameters in Kerr spacetime
• New Cataclysmic Variables and other Exotic Binaries in the Globular Cluster 47 Tucanae
• Pruning The ELM Survey: Characterizing Candidate Low-Mass White Dwarfs Through Photometric Variability
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• The Hills Mechanism and the Galactic Center S-stars
• Brownian motion of massive black hole binaries and the final parsec problem
• Planet-Mediated Precision-Reconstruction of the Evolution of the Cataclysmic Variable HU Aquarius
• Year 1 of the ZTF high-cadence Galactic Plane Survey: Strategy, goals, and early results on new single-mode hot subdwarf B-star pulsators
• Constraints on Black Hole/Host Galaxy Co-evolution and Binary Stalling Using Pulsar Timing Arrays
• Formation of sdB-stars via common envelope ejection by substellar companions
• Chasing the observational signatures of seed black holes at z > 7: candidate observability
• Chasing the observational signatures of seed black holes at z > 7: candidate statistics
• Negative Dynamical Friction on compact objects moving through dense gas
• The sustainable growth of the first black holes
• Listening to the gravitational wave sound of circumbinary exoplanets
• A Link Between Ram Pressure Stripping and Active Galactic Nuclei
• The LISA-Taiji network: precision localization of massive black hole binaries
• Second-order perturbation theory: the problem of infinite mode coupling
• Limits of Astrophysics with Gravitational-Wave Backgrounds
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations
• The formation and coalescence sites of the first gravitational wave events
• Eating Planets for Lunch and Dinner: Signatures of Planet Consumption by Evolving Stars
• Accretion in Strong Field Gravity with eXTP
• Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
• Colloquium: Comparison of Astrophysical and Terrestrial Frequency Standards
• Disks Around Merging Binary Black Holes: From GW150914 to Supermassive Black Holes
• Indication of Another Intermediate-mass Black Hole in the Galactic Center
• Search of sub-parsec massive binary black holes through line diagnosis
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• Gaseous Dynamical Friction in Presence of Black Hole Radiative Feedback
• A rapid evolving region in the Galactic Center: Why S-stars thermalize and more massive stars are missing
• Double Compact Objects as Low-frequency Gravitational Wave Sources
• Recent developments in planet migration theory
• Orbits in a non-Kerr Dynamical System
• Alternative LISA-TAIJI networks
• Gravitational tuning forks and hierarchical triple systems
• An ultracompact X-ray binary in the globular cluster NGC 1851
• Black Hole Starvation and Bulge Evolution in a Milky Way-like Galaxy
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• $N-$body dynamics of Intermediate mass-ratio inspirals in globular clusters
• SDSS1133: An Unusually Persistent Transient in a Nearby Dwarf Galaxy
• Growth of intermediate mass black holes by tidal disruption events in the first star clusters
• Glimmering in the dark: modeling the low-mass end of the $M_{\bullet }-\sigma$ relation and of the quasar luminosity function
• Repeated Imaging of Massive Black Hole Binary Orbits with Millimeter Interferometry: measuring black hole masses and the Hubble constant
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• The Process of Stellar Tidal Disruption by Supermassive Black Holes. The first pericenter passage
• Detecting extreme mass ratio inspirals with LISA using time-frequency methods
• Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources
• Young and turbulent: the early life of massive galaxy progenitors
• Phase shift of gravitational waves induced by aberration
• Compact massive objects in Virgo galaxies: the black hole population
• Double Neutron Star Formation: Merger Times, Systemic Velocities, and Travel Distances
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Black hole mergers: do gas discs lead to spin alignment?
• Infalling clouds on to supermassive black hole binaries - II. Binary evolution and the final parsec problem
• Non-local parameter degeneracy in the intrinsic space of gravitational-wave signals from extreme-mass-ratio inspirals
• Novel modelling of ultra-compact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars
• Radio-quiet and radio-loud pulsars: similar in Gamma-rays but different in X-rays
• Making massive stars in the Galactic Centre via accretion onto low-mass stars within an accretion disc
• Merger of white dwarf-neutron star binaries: Prelude to hydrodynamic simulations in general relativity
• Construction of the second-order gravitational perturbations produced by a compact object
• Stellar Energy Relaxation around A Massive Black Hole
• Exploring the unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291: the asynchronous growth of bulges and black holes
• Heavy double neutron stars: birth, mid-life and death
• A coherent acceleration search of the Parkes multi-beam pulsar survey - techniques and the discovery and timing of 16 pulsars
• Chandra X-rays from the redshift 7.54 quasar ULAS J1342+0928
• Milky Way Satellites Shining Bright in Gravitational Waves
• Dynamical Evolution and Merger Time-scales of LISA Massive Black Hole Binaries in Disk Galaxy Mergers
• Origin of supermassive black holes in massive metal-poor protoclusters
• Comment on "A non-interacting low-mass black hole -- giant star binary system"
• Boosted Tidal Disruption by Massive Black Hole Binaries During Galaxy Mergers FROM The View of N-Body Simulation
• High-Speed Photometry of Gaia14aae: An Eclipsing AM CVn That Challenges Formation Models
• Scalar Resonant Relaxation of Stars Around a Massive Black Hole
• The Response of Giant Stars To Dynamical-Timescale Mass Loss
• The z=7.54 Quasar ULAS J1342+0928 Is Hosted by a Galaxy Merger
• Galaxy formation with radiative and chemical feedback
• Galaxy Rotation and Supermassive Black Hole Binary Evolution
• Three-dimensional hydrodynamical models of wind and outburst-related accretion in symbiotic systems
• A Constrained Metropolis-Hastings Search for EMRIs in the Mock LISA Data Challenge 1B
• The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
• Close companions to Brightest Cluster Galaxies: Support for minor mergers and downsizing
• Gravitational Waves from Chaotic Dynamical System
• Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• AGN-starburst evolutionary connection : a physical interpretation based on radiative feedback
• Magnetorotational Collapse of Supermassive Stars: Black Hole Formation, Gravitational Waves and Jets
• The competing effect of gas and stars in massive black hole binaries evolution
• Relativistic dynamics of stars near a supermassive black hole
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• Detecting Kozai-Lidov imprints on the gravitational waves of intermediate-mass black holes in galactic nuclei
• Does GW190425 require an alternative formation pathway than a fast-merging channel?
• The Helium-Rich Cataclysmic Variable ES Ceti
• The mass assembly of high-redshift black holes
• The cataclysmic variable QZ Lib: a period bouncer
• Evolution of Retrograde Orbiters in an AGN Disk
• A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
• Emission Signatures from Sub-parsec Binary Supermassive Black Holes I: Diagnostic Power of Broad Emission Lines
• Prospects of eLISA for Detecting Galactic Binary Black Holes Similar to GW150914
• Was GW190412 born from a hierarchical 3+1 quadruple configuration?
• The history of the dark and luminous side of Milky Way-like progenitors
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- I. cataclysmic variables -- present-day population
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• The Emergence of the First Star-free Atomic Cooling Haloes in the Universe
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Toward the unambiguous identification of supermassive binary black holes through Bayesian inference
• EMRI data analysis with a phenomenological waveform
• Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
• Isotropic-Nematic Phase Transitions in Gravitational Systems
• Improved time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
• On the stability and collisions in triple stellar systems
• On the orbital periods of the AM CVn stars HP Librae and V803 Centauri
• Irradiation Pressure Effects in Close Binary Systems
• Consequences of Disk Scale Height on LISA Confusion Noise from Close White Dwarf Binaries
• Population Estimates for Electromagnetically-Distinguishable Supermassive Binary Black Holes
• Transformation of the multipolar components of gravitational radiation under rotations and boosts
• Black Hole Hunting with LISA
• Populating the Black Hole Mass Gaps In Stellar Clusters: General Relations and Upper Limits
• A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph
• Lack of nuclear clusters in dwarf spheroidal galaxies: implications for massive black holes formation and the cusp/core problem
• Infalling clouds onto super-massive black hole binaries - I. Formation of discs, accretion and gas dynamics
• Enhanced accretion rates of stars on Super-massive Black Holes by star-disk interactions in galactic nuclei
• The High Time Resolution Universe Pulsar Survey -- XVI. Discovery and timing of 40 pulsars from the southern Galactic plane
• Transient acceleration events in LISA Pathfinder data: properties and possible physical origin
• Blocking low-eccentricity EMRIs: A statistical direct-summation N-body study of the Schwarzschild barrier
• The influence of Massive Black Hole Binaries on the Morphology of Merger Remnants
• Post-Newtonian effects in N-body dynamics: Relativistic precession and conserved quantities in hierarchical triple systems
• LISA and the Existence of a Fast-Merging Double Neutron Star Formation Channel
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Multi-messenger-Athena Synergy White Paper
• The OmegaWhite Survey for Short-Period Variable Stars I: Overview and First Results
• A plethora of new R Coronae Borealis stars discovered from a dedicated spectroscopic follow-up survey
• Gas squeezing during the merger of a supermassive black hole binary
• Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation
• Extreme-mass-ratio-bursts from extragalactic sources
• On the eccentricity evolution of massive black hole binaries in stellar backgrounds
• General relativistic smoothed particle hydrodynamics
• Resolving the Complex Evolution of a Supermassive Black Hole Triplet in a Cosmological Simulation
• Swift data hint at a binary Super Massive Black Hole candidate at sub-parsec separation
• Constraining the neutron star equation of state using Pulse Profile Modeling
• The statistical mechanics of relativistic orbits around a massive black hole
• Automated bar detection in local disc galaxies from the SDSS - The colors of bars
• Using large spectroscopic surveys to test the double degenerate model for Type Ia supernovae
• LIGO/VIRGO searches for gravitational radiation in hypernovae
• Stellar Dynamics around a Massive Black Hole II: Resonant Relaxation
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
• Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
• Detection Strategies for Extreme Mass Ratio Inspirals
• XMM-Newton observations of AM CVn binaries
• Nonlinear dynamical tides in white dwarf binaries
• Testing general relativity using binary extreme-mass-ratio inspirals
• Neutrino and gravitational wave signal of a delayed-detonation model of Type Ia supernovae
• A 1201 s Orbital Period Detached Binary: the First Double Helium Core White Dwarf LISA Verification Binary
• The lifetime of binary black holes in Sérsic galaxy models
• Galaxy fields of LISA massive black hole mergers in a simulated Universe
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Emission Signatures from Sub-parsec Binary Supermassive Black Holes II: Effect of Accretion Disk Wind on Broad Emission Lines
• Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters
• Can supernova kicks trigger EMRIs in the Galactic Centre?
• Binary formation and mass function variations in fragmenting discs with short cooling times
• Hypervelocity Stars from a Supermassive Black Hole-Intermediate-mass Black Hole binary
• A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
• Expectations for extreme-mass-ratio bursts from the Galactic Centre
• SDSS J163030.58+423305.8: A 40 minute Orbital Period Detached White Dwarf Binary
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• Stars stripped in binaries -- the living gravitational wave sources
• Measuring Gas Accretion and Angular Momentum near Simulated Supermassive Black Holes
• Tidal Effects in Eccentric Coalescing Neutron Star Binaries
• Finding binary black holes in the Milky Way with LISA
• Vector Resonant Relaxation of Stars around a Massive Black Hole
• Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
• XMM-Newton observations of AM CVn binaries: V396 Hya & SDSS J1240-01
• Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
• Numerical Simulations of Equatorially-Asymmetric Magnetized Supernovae: Formation of Magnetars and Their Kicks
• Extreme recoils: impact on the detection of gravitational waves from massive black hole binaries
• Spatial dispersion of light rays propagating through a plasma in Kerr spacetime
• Improved gravitational radiation time-scales II: spin-orbit contributions and environmental perturbations
• Sowing black hole seeds: Direct collapse black hole formation with realistic Lyman-Werner radiation in cosmological simulations
• RApid Temporal Survey - RATS I: Overview and first results
• The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center
• Observational signatures of massive black hole formation in the early universe
• Multi-band gravitational wave astronomy: science with joint space- and ground-based observations of black hole binaries
• Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies
• Search of sub-parsec massive binary black holes through line diagnosis II
• Revisiting dynamical friction: the role of global modes and local wakes
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• The OmegaWhite survey for short-period variable stars - V. Discovery of an ultracompact hot subdwarf binary with a compact companion in a 44 minute orbit
• Secular dynamics of binaries in stellar clusters I: general formulation and dependence on cluster potential
• Inward Bound: The incredible journey of massive black holes as they pair and merge; I. The effect of mass ratio in flattened rotating galactic nuclei
• The Binding Energy Parameter for Common Envelope Evolution
• Circumbinary disc self-gravity governing supermassive black hole binary mergers
• Bar resilience to flybys in a cosmological framework
• Expected intermediate-mass black holes in the Virgo cluster. I. Early-type galaxies
• Evolution Of Binary Supermassive Black Holes In Rotating Nuclei
• Is there an intermediate massive black hole in the Galactic center: Imprints on the stellar tidal-disruption rate
• Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations
• Compact object binary mergers driven by cluster tides: a new channel for LIGO/Virgo gravitational wave events
• Tidal disruption events in the first billion years of a galaxy
• Pulsar timing in extreme mass ratio binaries: a general relativistic approach
• The Turn-On of Mass Transfer in AM CVn Binaries: Implications for RX J0806+1527 and RX J1914+2456
• Estimating the outcomes of common envelope evolution in triple stellar systems
• The effect of AGN feedback on the migration timescale of supermassive black holes binaries
• SDSS J1056+5516: A Triple AGN or an SMBH Recoil Candidate?
• Ultra-compact X-ray binaries as dual-line gravitational-wave sources
• Prospects of gravitational-waves detections from common-envelope evolution with LISA
• Super massive black holes in star forming gaseous circumnuclear discs
• A Potential Recoiling Supermassive Black Hole CXO J101527.2+625911
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks
• Measuring tides and binary parameters from gravitational wave data and eclipsing timings of detached white dwarf binaries
• The butterfly effect in the extreme-mass ratio inspiral problem
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Effects of non-Kozai mutual inclinations on two-planet system stability through all phases of stellar evolution
• Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna
• Hydrodynamics of Coalescing Binary Neutron Stars: Ellipsoidal Treatment
• Accuracy of the post-Newtonian approximation. II. Optimal asymptotic expansion of the energy flux for quasicircular, extreme mass-ratio inspirals into a Kerr black hole
• Massive black hole binary plane reorientation in rotating stellar systems
• Detecting extreme mass ratio inspiral events in LISA data using the Hierarchical Algorithm for Clusters and Ridges (HACR)
• Constraining parameters of white-dwarf binaries using gravitational-wave and electromagnetic observations
• Phase resolved spectroscopy and Kepler photometry of the ultracompact AM CVn binary SDSS J190817.07+394036.4
• Dynamical friction-driven orbital circularisation in rotating discs: a semi-analytical description
• Orbital Evolution of Neutron-Star -- White-Dwarf Binaries by Roche-Lobe Overflow and Gravitational Wave Radiation
• Gravitational Wave Driven Mergers and Coalescence Time of Supermassive Black Holes
• The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture
• Pairing of Massive Black Holes in Merger Galaxies Driven by Dynamical Friction
• Demographics of triple systems in dense star clusters
• On the formation of hot and warm Jupiters via secular high-eccentricity migration in stellar triples
• Prospects for Gravitational Wave Measurement of ZTFJ1539+5027
• How to detect the shortest-period binary pulsars in the era of LISA
• The Milky Way's bar structural properties from gravitational waves
• Gravitational Encounters and the Evolution of Galactic Nuclei. I. Method
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory
• Prospects for observing ultra-compact binaries with space-based gravitational wave interferometers and optical telescopes
• New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations
• On the orbital properties of millisecond pulsar binaries
• Star cluster disruption by a massive black hole binary
• Observable gravitational waves from tidal disruption events and their electromagnetic counterpart
• Detectability of modulated X-rays from LISA's supermassive black hole mergers
• Tidal disruption event rates in galaxy merger remnants
• The gravitational wave background signal from tidal disruption events
• A universal minimal mass scale for present-day central black holes
• Bondi-Hoyle-Lyttleton accretion by binary stars
• Relativistic mergers of compact binaries in clusters: The fingerprint of the spin
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Exciting modes due to the aberration of gravitational waves: Measurability for extreme-mass-ratio inspirals
• Using electromagnetic observations to aid gravitational-wave parameter estimation of compact binaries observed with LISA II: The effect of knowing the sky position
• How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
• Searching for Intermediate Mass Black Holes in galaxies with Low Luminosity AGN: A multiple-method approach
• Fast Spinning Pulsars as Probes of Massive Black Holes' Gravity
• Isotropic-Nematic Phase Transitions in Gravitational Systems II: Higher Order Multipoles
• A 15.7-Minute AM CVn Binary Discovered in K2
• Discovery of the first resolved triple white dwarf
• The role of bars on the dynamical-friction driven inspiral of massive perturbers
• Gravitational Waves from Global Second Order Phase Transitions
• Emission Signatures from Sub-parsec Binary Supermassive Black Holes III: Comparison of Models with Observations
• Tidal Perturbations to the Gravitational Inspiral of J0651+2844
• The chemical composition of the accretion disk and donor star in Ultra Compact X-ray Binaries: A comprehensive X-ray analysis
• Cosmic archaeology with massive stellar black hole binaries
• The Carnegie Supernova Project II. Observations of the luminous red nova AT 2014ej
• How bright are the gaps in circumbinary disk systems?
• Weighing Milky Way Satellites with LISA
• Gravitational waves from dynamical tides in white dwarf binaries
• Spin dynamics of a millisecond pulsar orbiting closely around a massive black hole
• Discovery of a high state AM CVn binary in the Galactic Bulge Survey
• Black hole spin evolution in warped accretion discs
• Time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
• Double Neutron Stars: Evidence For Two Different Neutron-Star Formation Mechanisms
• On Spin Dependence of the Fundamental Plane of Black Hole Activity
• Golden galactic binaries for LISA: mass-transferring white dwarf black hole binaries
• Likelihood for Detection of Sub-parsec Supermassive Black Hole Binaries in Spectroscopic Surveys
• The black hole retention fraction in star clusters
• The gravitational capture of compact objects by massive black holes
• LISA sources from young massive and open stellar clusters
• Galaxies with monstrous black holes in galaxy cluster environments
• On the maximum accretion rate of supermassive stars
• Evolution of Low-Mass X-ray Binaries: the Effect of Donor Evaporation
• High-Mass X-ray Binaries: progenitors of double compact objects
• Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence
• Formation constraints indicate a black-hole accretor in 47 Tuc X9
• Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
• Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters
• On the maximum stellar rotation to form a black hole without an accompanying luminous transient
• Stellar variability on time-scales of minutes: results from the first 5 years of the Rapid Temporal Survey (RATS)
• Bayesian inference on EMRI signals using low frequency approximations
• Evolution of dwarf galaxies hosting GW150914-like events
• Electromagnetic emission of white dwarf binary mergers
• Gravitational waves from tidal disruption events: an open and comprehensive catalogue
• The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach
• Automatic Bayesian inference for LISA data analysis strategies
• The torquing of circumnuclear accretion disks by stars and the evolution of massive black holes
• Non-isotropic feedback from accreting spinning black holes
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
• Binaries Wandering Around Supermassive Black Holes Due To Gravito-electromagnetism
• Cosmological Physics with Black Holes (and Possibly White Dwarfs)
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• External Enrichment of Minihalos by the First Supernovae
• Search for Neutron Star Binaries in the Local Group Galaxies Using LISA
• Constraining white dwarf viscosity through tidal heating in detached binary systems
• Common Envelope Wind Tunnel: Range of Applicability and Self-Similarity in Realistic Stellar Envelopes
• Simulating the Magnetorotational Collapse of Supermassive Stars: Incorporating Gas Pressure Perturbations and Different Rotation Profiles
• An ancient double degenerate merger in the Milky Way halo
• The evolution of a binary in a retrograde circular orbit embedded in an accretion disk
• Gravitational wave emission from unstable accretion discs in tidal disruption events
• Large-scale structures in the $\Lambda$CDM Universe: network analysis and machine learning
• A Gemini Snapshot Survey for Double Degenerates
• Ultra-relativistic astrophysics using multi-messenger observations of double neutron stars with LISA and the SKA
• Composition of an Emission Line System in Black Hole Host Globular Cluster RZ2109
• Orbital period variation of KIC 10544976: Applegate mechanism versus light travel time effect
• Gravitational Wave Emission from the Single-Degenerate Channel of Type Ia Supernovae
• Dynamical evolution of massive perturbers in realistic multi-component galaxy models I: implementation and validation
• Massive Star Formation in Metal-Enriched Haloes at High Redshift
• Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
• Estimating the fossil disc mass during supermassive black hole mergers: the importance of torque implementation
• A Second Decoupling Between Merging Binary Black Holes and the Inner Disc--Impact on the Electromagnetic Counterpart
• The strong environmental dependence of black hole scaling relations
• Sparse data inpainting for the recovery of Galactic-binary gravitational wave signals from gapped data
• Non-linear effects in EMRI dynamics and their imprints on gravitational waves
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• Orbital spin dynamics of a millisecond pulsar around a massive black hole with an general mass quadrupole
• The role of gravitational recoil in the assembly of massive black hole seeds
• Complex orbital dynamics of a double neutron star system revolving around a massive black hole
• Binary white dwarfs in the halo of the Milky Way
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Search for a stochastic gravitational-wave signal in the second round of the Mock LISA Data Challenges
• On the possibility of detecting ultra-short period exoplanets with LISA
• How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
• Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors
• CHANDRA Detection of the AM CVn binary ES Cet (KUV 01584-0939)
• Black hole and nuclear cluster scaling relations: M_bh ~ M_nc^{2.7+/-0.7}
• Supermassive black hole spin-flip during the inspiral
• Evolution of inspiralling neutron star binaries: effects of tidal interactions and orbital eccentricities
• Radiation-Reaction Force on a Small Charged Body to Second Order
• Intermediate mass black holes' effect on compact object binaries
• Tidal torque induced by orbital decay in compact object binaries
• The Evolution of Kicked Stellar-Mass Black Holes in Star Cluster Environments
• Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo
• Determining the nature of white dwarfs from low-frequency gravitational waves
• Verifying black hole orbits with gravitational spectroscopy
• The Pairing Probability of Massive Black Holes in Merger Galaxies in the Presence of Radiative Feedback
• An Efficient Signal to Noise Approximation for Eccentric Inspiraling Binaries
• The Abundance of X-Shaped Radio Sources: Implications for the Gravitational Wave Background
• A far-ultraviolet variable with an 18-minute period in the globular cluster NGC 1851
• Slow Decline and Rise of the Broad [OIII] Emission Line in Globular Cluster Black Hole Candidate RZ2109
• Time-resolved X-Shooter spectra and RXTE light curves of the ultra-compact X-ray binary candidate 4U 0614+091
• A Markov Chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei
• Connecting traces of galaxy evolution: the missing core mass -- morphological fine structure relation
• On the detectability of ultra-compact binary pulsar systems
• Minimum Orbital Periods of H-Rich Bodies
• Tidal disruption rates in non-spherical galactic nuclei formed by galaxy mergers
• A Statistical Method to Search for Recoiling Supermassive Black Holes in Active Galactic Nuclei
• MOCCA-Survey Database: Extra Galactic Globular Clusters. II. Milky Way and Andromeda
• Real galaxy mergers from galaxy pair catalogs
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Gravitational Burst Radiation from Pulsars in the Galactic centre and stellar clusters
• Analytic Approximations in GR and Gravitational Waves
• The X-ray variable sky as seen by MAXI: the future of dust echo tomography with bright Galactic X-ray bursts
• Accretion of clumpy cold gas onto massive black holes binaries: the challenging formation of extended circumbinary structures
• Will Gravitational Waves Discover the First Extra-Galactic Planetary System?
• Large Scale Searches for Brown Dwarfs and Free-Floating Planets
• Periodicities in the K2 lightcurve of HP Librae
• The most massive galaxies with large depleted cores: structural parameter relations and black hole masses

Cited by in corpus (2)

• The NewAthena mission concept in the context of the next decade of X-ray astronomy
• Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies