Characterization of the LIGO detectors during their sixth science run

Abstract

In 2009-2010, the Laser Interferometer Gravitational-wave Observa- tory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves of astrophysical origin. The sensitiv- ity of these detectors was limited by a combination of noise sources inherent to the instrumental design and its environment, often localized in time or frequency, that couple into the gravitational-wave readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the de- tectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of LIGO to a variety of astrophysical sources.

arXiv comment31 pages, 13 figures

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• State of the field: Binary black hole natal kicks and prospects for isolated field formation after GWTC-2
• Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• The final core collapse of pulsational pair instability supernovae
• Parameter estimation for gravitational-wave bursts with the BayesWave pipeline
• Subtraction of correlated noise in global networks of gravitational-wave interferometers
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
• Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
• Primordial gravitational waves and the H0-tension problem
• Testing the multipole structure of compact binaries using gravitational wave observations
• Testing Einstein's Weak Equivalence Principle With Gravitational Waves
• When will we observe binary black holes precessing?
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Improving gravitational-wave parameter estimation using Gaussian process regression
• Capturing the electromagnetic counterparts of binary neutron star mergers through low latency gravitational wave triggers
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and post-adiabatic corrections
• Resolving The Peak Of The Black Hole Mass Spectrum
• Teamwork Makes the Dream Work: Optimizing Multi-Telescope Observations of Gravitational-Wave Counterparts
• GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam
• Modelling the Ringdown from Precessing Black Hole Binaries
• Deep Learning Ensemble for Real-time Gravitational Wave Detection of Spinning Binary Black Hole Mergers
• Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910
• Gravitational wave detectors with broadband high frequency sensitivity
• Time-Frequency Analysis of Gravitational Wave Data
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• A new data analysis framework for the search of continuous gravitational wave signals
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions
• Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries
• A Machine Learning Based Source Property Inference for Compact Binary Mergers
• Enabling high confidence detections of gravitational-wave bursts
• Leveraging waveform complexity for confident detection of gravitational waves
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• On the identification of individual gravitational wave image types of a lensed system using higher-order modes
• The host galaxies of double compact objects merging in the local Universe
• Detection of astrophysical gravitational wave sources by TianQin and LISA
• The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory
• Constraints on primordial curvature spectrum from primordial black holes and scalar-induced gravitational waves
• On the detectability of ultralight scalar field dark matter with gravitational-wave detectors
• Quantifying the Effect of Power Spectral Density Uncertainty on Gravitational-Wave Parameter Estimation for Compact Binary Sources
• Maximum redshift of gravitational wave merger events
• Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei
• Accuracy of binary black hole waveform models for aligned-spin binaries
• Search for a scalar induced stochastic gravitational wave background in the third LIGO-Virgo observing run
• Standard-siren cosmology using gravitational waves from binary black holes
• Removing degeneracy and multimodality in gravitational wave source parameters
• Observation of a Correlation Between Internal friction and Urbach Energy in Amorphous Oxides Thin Films
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
• Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
• Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
• Improvements to the construction of binary black hole initial data
• Cosmology with Standard Sirens at Cosmic Noon
• Search for gravitational waves from the coalescence of sub-solar mass and eccentric compact binaries
• Adding eccentricity to quasicircular binary-black-hole waveform models
• Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches
• X-ray-powered macronovae
• On the interpretation of the Fermi GBM transient observed in coincidence with LIGO Gravitational Wave Event GW150914
• Detection Prospects of Core-Collapse Supernovae with Supernova-Optimized Third-Generation Gravitational-wave Detectors
• Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
• Optimization of seismometer arrays for the cancellation of Newtonian noise from seismic body waves
• Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey
• Spectral analysis of gravitational waves from binary neutron star merger remnants
• Hierarchical multi-stage MCMC follow-up of continuous gravitational wave candidates
• Robust semicoherent searches for continuous gravitational waves with noise and signal models including hours to days long transients
• Application of dictionary learning to denoise LIGO's blip noise transients
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• A compact, large-range interferometer for precision measurement and inertial sensing
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run
• Phase shift of gravitational waves induced by aberration
• Identifying when Precession can be Measured in Gravitational Waveforms
• Flexible and Fast Estimation of Binary Merger Population Distributions with Adaptive KDE
• Gravitational-wave inference in the catalog era: evolving priors and marginal events
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Towards a first design of a Newtonian-noise cancellation system for Advanced LIGO
• Implications of dedicated seismometer measurements on Newtonian-noise cancellation for Advanced LIGO
• $N-$body dynamics of Intermediate mass-ratio inspirals in globular clusters
• The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
• Parametrized tests of post-Newtonian theory using principal component analysis
• Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Limits on hierarchical black hole mergers from the most negative ${\chi }_{\mathrm{eff}}$ systems
• Pre-merger localization of compact-binary mergers with third generation observatories
• GW170817A as a Hierarchical Black Hole Merger
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• Bayesian nonparametric spectral density estimation using B-spline priors
• Spin it as you like: the (lack of a) measurement of the spin tilt distribution with LIGO-Virgo-KAGRA binary black holes
• Heavy double neutron stars: birth, mid-life and death
• Using Deep Learning to Localize Gravitational Wave Sources
• Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
• Ultrahigh frequency primordial gravitational waves beyond the kHz: The case of cosmic strings
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• High-Reflection Coatings for Gravitational-Wave Detectors: State of The Art and Future Developments
• Very fast stochastic gravitational wave background map making using folded data
• Newtonian-noise cancellation in full-tensor gravitational-wave detectors
• Prospects for joint gravitational wave and short gamma-ray burst observations
• Spectroscopic analysis of stellar mass black-hole mergers in our local universe with ground-based gravitational wave detectors
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission
• The orbit of GW170817 was inclined by less than 28 degrees to the line of sight
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• A comparison of methods for the detection of gravitational waves from unknown neutron stars
• Second Einstein Telescope Mock Data and Science Challenge: Low Frequency Binary Neutron Star Data Analysis
• Tiling strategies for optical follow-up of gravitational wave triggers by wide field of view telescopes
• Evolution of Retrograde Orbiters in an AGN Disk
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Detecting the Beaming Effect of Gravitational Waves
• Fusing numerical relativity and deep learning to detect higher-order multipole waveforms from eccentric binary black hole mergers
• Primordial gravitational waves in Horndeski gravity
• Evidence for the evolution of black hole mass function with redshift
• Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail
• Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data
• Improving the background of gravitational-wave searches for core collapse supernovae: A machine learning approach
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Improved statistic to identify strongly lensed gravitational wave events
• High-power all-fiber ultra-low noise laser
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• Merger rate of stellar black hole binaries above the pair instability mass gap
• R-mode astronomy
• All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
• Simple procedures to reduce eccentricity of binary black hole simulations
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Utilizing aLIGO Glitch Classifications to Validate Gravitational-Wave Candidates
• X-ray guided gravitational-wave search for binary neutron star merger remnants
• The initial value problem as it relates to numerical relativity
• Passive, free-space laser gyroscope
• Searching for anisotropy in the distribution of binary black hole mergers
• Multiband Gravitational Wave Parameter Estimation: A Study of Future Detectors
• Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project
• The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source
• Systematic errors in estimation of gravitational-wave candidate significance
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• Search for Continuous Gravitational Waves from the Central Compact Objects in Supernova Remnants Cassiopeia A, Vela Jr. and G347.3-0.5
• Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei
• Excitation of f-modes during mergers of spinning binary neutron star
• Neutron star binary orbits in their host potential: effect on early r-process enrichment
• All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• lensingGW: a Python package for lensing of gravitational waves
• SOAP: A generalised application of the Viterbi algorithm to searches for continuous gravitational-wave signals
• Numerical investigation of plasma-driven superradiant instabilities
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries
• The host galaxies of double compact objects across cosmic time
• Constraining early dark energy with gravitational waves before recombination
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• New equation of states for postmerger supramassive quark stars
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• Probing new light gauge bosons with gravitational-wave interferometers using an adapted semi-coherent method
• Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
• Control strategy to limit duty cycle impact of earthquakes on the LIGO gravitational-wave detectors
• All-sky search for long-duration gravitational wave transients with LIGO
• Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
• Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
• Joint search for isolated sources and an unresolved confusion background in pulsar timing array data
• High Quality QCD Axion at Gravitational Wave Observatories
• Black Hole Leftovers: The Remnant Population from Binary Black Hole Mergers
• Globally coherent short duration magnetic field transients and their effect on ground based gravitational-wave detectors
• Measuring stochastic gravitational-wave energy beyond general relativity
• Systematic errors in estimation of gravitational-wave candidate significance
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• Effect of spin on the inspiral of binary neutron stars
• Bayesian Multi-Messenger Search Method for Common Sources of Gravitational Waves and High-Energy Neutrinos
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Euclid: Superluminous supernovae in the Deep Survey
• Primordial Black Holes from Conformal Higgs
• Assessing the compact-binary merger candidates reported by the MBTA pipeline in the LIGO-Virgo O3 run: probability of astrophysical origin, classification, and associated uncertainties
• Characterizing Earth gravity field fluctuations with the MIGA antenna for future Gravitational Wave detectors
• Anomaly Detection in Gravitational Waves data using Convolutional AutoEncoders
• Stars stripped in binaries -- the living gravitational wave sources
• Searches for continuous gravitational waves from Scorpius X-1 and XTE J1751-305 in LIGO's sixth science run
• Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
• Detecting gravitational-wave transients at five sigma: a hierarchical approach
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Probing hybrid stars with gravitational waves via interfacial modes
• Gravitational wave signatures of PBH-generated baryon-dark matter coincidence
• Gravitational Waves from Core-Collapse Supernovae
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• LSTM and CNN application for core-collapse supernova search in gravitational wave real data
• The next detectors for gravitational wave astronomy
• Sub-threshold binary neutron star search in Advanced LIGO's first observing run
• Improving LIGO calibration accuracy by tracking and compensating for slow temporal variations
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Constraint on the ejecta mass for a black hole-neutron star merger event candidate S190814bv
• Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields
• The quasi normal modes of growing dirty black holes
• Gamma-Ray Flashes from Dark Photons in Neutron Star Mergers
• Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence
• Probing elastic quark phases in hybrid stars with radius measurements
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Petrov Type, Principal Null Directions, and Killing Tensors of Slowly-Rotating Black Holes in Quadratic Gravity
• Frequency-domain waveform approximants capturing Doppler shifts
• Searching for parity violation with the LIGO-Virgo-KAGRA network
• Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Reducing the effect of seismic noise in LIGO searches by targeted veto generation
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• Total-variation methods for gravitational-wave denoising: performance tests on Advanced LIGO data
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• Characterizing the observation bias in gravitational-wave detections and finding structured population properties
• A robust machine learning algorithm to search for continuous gravitational waves
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Can we decipher the composition of the core of a neutron star?
• Material Size Dependence on Fundamental Constants
• Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• Model exploration in gravitational-wave astronomy with the maximum population likelihood
• Astrophysical Gravitational-Wave Echoes from Galactic Nuclei
• Observing Gravitational Waves with a Single Detector
• Limiting the effects of earthquakes on gravitational-wave interferometers
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Quantum interactions between a laser interferometer and gravitational waves
• Pinning down the primordial black hole formation mechanism with gamma-rays and gravitational waves
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1
• First Tests of a Newtonian Calibrator on an Interferometric Gravitational Wave Detector
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• Modeling gravitational waves from exotic compact objects
• Identification of Binary Neutron Star Mergers in Gravitational-Wave Data Using YOLO One-Shot Object Detection
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• Gravitational-wave echoes from numerical-relativity waveforms via space-time construction near merging compact objects
• A search for radio emission from double-neutron star merger GW190425 using Apertif
• Observing binary black hole ringdowns by advanced gravitational wave detectors
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• The String Soundscape at Gravitational Wave Detectors
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• The first five years of gravitational-wave astrophysics
• Presto-Color: A Photometric Survey Cadence for Explosive Physics & Fast Transients
• The short gamma-ray burst population in a quasi-universal jet scenario
• Detecting the stochastic gravitational wave background with the TianQin detector
• Characterization of numerical relativity waveforms of eccentric binary black hole mergers
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• A search of the Orion spur for continuous gravitational waves using a "loosely coherent" algorithm on data from LIGO interferometers
• Gravitational wave detection without boot straps: a Bayesian approach
• Gravitational waves from melting cosmic strings
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• A search for the afterglows, kilonovae, and host galaxies of two short GRBs: GRB 211106A and GRB 211227A
• Gravitational wave probes of particle dark matter: a review
• Observational Selection Effects with Ground-based Gravitational Wave Detectors
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Time-dependent stellar-mass binary black hole mergers in AGN disks: Mass distribution of hierarchical mergers
• Speedmeter scheme for gravitational-wave detectors based on EPR quantum entanglement
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• The payload of the Lunar Gravitational-wave Antenna
• Local-Oscillator Noise Coupling in Balanced Homodyne Readout for Advanced Gravitational Wave Detectors
• Seismic array measurements at Virgo's West End Building for the configuration of a Newtonian-noise cancellation system
• The Kitt Peak Electron Multiplying CCD demonstrator
• Technology for the next gravitational wave detectors
• A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing Runs
• Distinguishing binary neutron star from neutron star-black hole mergers with gravitational waves
• Estimation of starting times of quasinormal modes in ringdown gravitational waves with the Hilbert-Huang transform
• Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression
• GWitchHunters: Machine Learning and citizen science to improve the performance of Gravitational Wave detector
• The reliability of the low-latency estimation of binary neutron star chirp mass
• High-accuracy simulations of highly spinning binary neutron star systems
• Mirror actuation design for the interferometer control of the KAGRA gravitational wave telescope
• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• Generalized uncertainty principle in resonant detectors of gravitational waves
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• On the rate and on the gravitational wave emission of short and long GRBs
• The KAGRA underground environment and lessons for the Einstein Telescope
• Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectors
• Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study
• First results and future prospects for dual-harmonic searches for gravitational waves from spinning neutron stars
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Quantum limited measurements with lossy optical cavity enabled by dissipative optomechanical coupling
• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• Faster search for long gravitational-wave transients: GPU implementation of the transient F-statistic
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• Counting on Short Gamma-Ray Bursts: Gravitational-Wave Constraints of Jet Geometry
• Swift-XRT Follow-up of Gravitational Wave Triggers in the Second Advanced LIGO/Virgo Observing Run
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Phase decoherence of gravitational wave backgrounds
• Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
• Understanding binary neutron star collisions with hypermodels
• Primordial black holes in scalar field inflation coupled to the Gauss-Bonnet term with fractional power-law potentials
• Fundamental quantum limits of multi-carrier optomechanical sensors
• Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
• Analytic Waveforms for Eccentric Gravitational Wave Bursts
• Investigation of magnetic noise in Advanced Virgo
• Probing neutron star structure via f-mode oscillations and damping in dynamical spacetime models
• A classifier for gravitational-wave inspiral signals in non-ideal single-detector data
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Compact intermediate-mass black hole X-ray binaries: potential LISA sources?
• Virgo Detector Characterization and Data Quality: tools
• Testing the Kerr nature of intermediate-mass and supermassive black hole binaries using spin-induced multipole moment measurements
• Ancestral Black Holes of Binary Merger GW190521
• Gravitational Waves from Phase Transition in Minimal SUSY $U(1{)}_{B-L}$ Model
• Speed of sound in dense matter and two families of compact stars
• Exact one-loop false vacuum decay rate
• Gravitational waves from pulsars with measured braking index
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Timing-residual power spectrum of a polarized stochastic gravitational-wave background in pulsar-timing-array observation
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Convolutional neural network for gravitational-wave early alert: Going down in frequency
• Post-merger chirps from binary black holes as probes of the final black-hole horizon
• Optimising the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
• Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger
• Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
• Search for Black Hole Merger Families
• Collapsing domain walls beyond $Z_2$
• Light Deflection Angle by Superentropic Black Holes
• XMM-Newton Slew Survey observations of the gravitational wave event GW150914
• A unified approach to ${\chi }^2$ discriminators for searches of gravitational waves from compact binary coalescences
• Towards mitigating the effect of sine-Gaussian noise transients on searches for gravitational waves from compact binary coalescences
• Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
• Active platform stabilisation with a 6D seismometer
• Post-inflationary thermal histories and the refractive index of relic gravitons
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• Matter Effects on LIGO/Virgo Searches for Gravitational Waves from Merging Neutron Stars
• Binary Black Hole Merger Rates Inferred from Luminosity Function of Ultra-Luminous X-ray Sources
• No evidence that the binary black hole mass distribution evolves with redshift
• GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes
• Inferring Parameters of GW170502: The Loudest Intermediate-mass Black Hole Trigger in LIGO's O1/O2 data
• Constraining domain wall dark matter with a network of superconducting gravimeters and LIGO
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Rapidly rotating neutron star progenitors
• Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
• Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis
• Modeling Mergers of Known Galactic Systems of Binary Neutron Stars
• Liverpool Telescope follow-up of candidate electromagnetic counterparts during the first run of Advanced LIGO
• Heavy dark matter and Gravitational waves
• Evidence for gravitational-wave dominated emission in the central engine of short GRB 200219A
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Tackling excess noise from bilinear and nonlinear couplings in gravitational-wave interferometers
• Footprints of population III stars in the gravitational-wave background
• Application of the third RIT binary black hole simulations catalog to parameter estimation of gravitational waves signals from the LIGO-Virgo O1/O2 observational runs
• What if GW190425 did not produce a black hole promptly?
• Multi-messenger astronomy of gravitational-wave sources with flexible wide-area radio transient surveys
• LISA Telescope: Phase noise due to pointing jitter
• Enhancing the significance of gravitational wave bursts through signal classification
• Ground-state cooling of dispersively coupled optomechanical system in unresolved sideband regime via dissipatively coupled oscillator
• Ground motion prediction at gravitational wave observatories using archival seismic data
• Dark Matter Induced Brownian Motion
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Detecting compact galactic binaries using a hybrid swarm-based algorithm
• Constraining binary mergers in AGN disks using the non-observation of lensed gravitational waves
• Feasibility of near-unstable cavities for future gravitational wave detectors
• Towards observing the neutron star collapse with gravitational wave detectors
• Power coupling losses for misaligned and mode-mismatched higher-order Hermite-Gauss modes
• Search for Gravitational Waves from Scorpius X-1 in LIGO O3 Data With Corrected Orbital Ephemeris
• How would GW150914 look with future GW detector networks?
• Searching for high-frequency gravitational waves by ground high field magnetic resonant sweepings
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• The Influence of Dual-Recycling on Parametric Instabilities at Advanced LIGO
• Search for Advanced LIGO Single Interferometer Compact Binary Coalescence Signals in Coincidence with Gamma-Ray Events in Fermi-GBM
• Unveiling the Nature of Gravitational-Wave Emission in Core-collapse Supernovae with Perturbative Analysis
• Search setup for long-duration transient gravitational waves from glitching pulsars during LIGO-Virgo third observing run
• Thermal charge carrier driven noise in transmissive semiconductor optics
• Bilinear noise subtraction at the GEO 600 observatory
• Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
• Microlensing bias on the detection of strong lensing gravitational wave
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• Gravitational wave detection from OJ 287 via a pulsar timing array
• Resonant amplification of curvature perturbations in inflation model with periodical derivative coupling
• Optical and mechanical properties of ion-beam-sputtered MgF${}_2$ thin films for gravitational-wave interferometers
• Thermal modelling of Advanced LIGO test masses
• Multi-messenger prospects for black hole - neutron star mergers in the O4 and O5 runs
• Boosting the sensitivity of high frequency gravitational wave detectors by PT-symmetry
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• The Murchison Widefield Array Transients Survey (MWATS). A search for low frequency variability in a bright Southern hemisphere sample
• Observational implications of lowering the LIGO-Virgo alert threshold
• A Quark-Nova in the wake of a core-collapse Supernova: a unifying model for long duration Gamma-Ray Bursts and Fast Radio Bursts
• Inconsistent black hole kick estimates from gravitational-wave models
• Exploring a search for long-duration transient gravitational waves associated with magnetar bursts
• Chasing 5-sigma: Prospects for searches for long-duration gravitational-waves without time slides
• Probing nuclear physics with supernova gravitational waves and machine learning
• Exclusion of standard $\hslash \omega$ gravitons by LIGO observation
• Constraining hierarchical mergers of binary black holes detectable with LIGO-Virgo
• Effects of mixing and annealing on the optical and mechanical properties of TiO${}_2$:Ta${}_2$O${}_5$ amorphous coatings
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• A stochastic template bank for gravitational wave searches for precessing neutron-star--black-hole coalescence events
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Variability in Short Gamma-ray Bursts: Gravitationally Unstable Tidal Tails
• Optical Gravitational Wave Antenna with Increased Power Handling Capability
• Gravitational wave emission from dynamical stellar interactions
• Short Gamma-Ray Bursts and Gravitational-Wave Observations from Eccentric Compact Binaries
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• Optimal Optical Search Strategy for Finding Transient in Large Sky Error Region Under Realistic Constraints
• Multi-messenger astronomy with INTEGRAL
• The optical loss study of molecular layer for a cryogenic interferometric gravitational-wave detector
• Source localizations with the network of space-based gravitational wave detectors
• Scalar Tops and Perturbed Quadrupoles: Probing Fundamental Physics with Spin-Precessing Binaries
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors
• Leptogenesis, Dark Matter and Gravitational Waves from Discrete Symmetry Breaking
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• Method to detect gravitational waves from an ensemble of known pulsars
• A hybrid silicon-sapphire cryogenic Fabry-Perot cavity using hydroxide catalysis bonding
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• Feasibility study of beam-expanding telescopes in the interferometer arms for the Einstein Telescope
• The imprint of superradiance on hierarchical black hole mergers
• An optimal ${\chi }^2$ discriminator against modelled noise-transients in interferometric data in searches for binary black-hole mergers
• J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
• Evidence for the transition of a Jacobi ellipsoid into a Maclaurin spheroid in gamma-ray bursts
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• A convolutional neural network to distinguish glitches from minute-long gravitational wave transients
• A time domain experiment with Swift: monitoring of seven nearby galaxies
• Numerically modeling Brownian thermal noise in amorphous and crystalline thin coatings
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
• Effects of proper motion of neutron stars on continuous gravitational-wave searches
• Quantum coherence of relic gravitons and Hanbury Brown-Twiss interferometry
• Matched-filter study and energy budget suggest no detectable gravitational-wave 'extended emission' from GW170817
• Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers
• Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role
• How to search for multiple messengers -- a general framework beyond two messengers
• Estimation of the gravitational wave polarizations from a non template search
• Accelerated detection of the binary neutron star gravitational-wave background
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• Fundamental Physics and Cosmology with TianQin
• Scalar polarization window in gravitational-wave signals
• Optimizing StackSlide setup and data selection for continuous-gravitational-wave searches in realistic detector data
• RATIR Followup of LIGO/Virgo Gravitational Wave Events
• Where binary neutron stars merge: predictions from IllustrisTNG
• Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits
• Topology change and emergent scale symmetry in compact star matter via gravitational wave detection
• The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range
• Dependence of the amplitude of gravitational waves from preheating on the inflationary energy scale
• Broadband Dichromatic Variational Measurement
• Evaporating black holes: constraints on anomalous emission mechanisms
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• Employing Deep Learning for Detection of Gravitational Waves from Compact Binary Coalescences
• Tracking Down the Route to the SM with Inflation and Gravitational Waves
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Gravitational waves and monopoles dark matter from first-order phase transition
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Study on electro-optic noise in crystalline coatings toward future gravitational wave detectors
• Memory Effect of Gravitational Wave Pulses in PP-Wave Spacetimes
• Implications of Pulsar Timing Array Results for High Frequency Gravitational Waves
• The binary black hole explorer: on-the-fly visualizations of precessing binary black holes
• HERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter
• Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field
• Projections of the uncertainty on the compact binary population background using popstock
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• Reducing the number of templates for aligned-spin compact binary coalescence gravitational wave searches using metric-agnostic template nudging
• Effects of transients in LIGO suspensions on searches for gravitational waves
• On the large apparent black hole spin-orbit misalignment angle in GW200115
• How close can we approach the event horizon of the Kerr black hole from the detection of the gravitational quasinormal modes?
• Search for the optical counterpart of the GW170814 gravitationalwave event with the VLT Survey Telescope
• Effect of Scalar Boson on Fermionic Dark Star
• All-sky Search for Periodic Gravitational Waves in the O1 LIGO Data
• A back-linked Fabry-Perot interferometer for space-borne gravitational wave observations
• No Glitch in the Matrix: Robust Reconstruction of Gravitational Wave Signals Under Noise Artifacts
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Toward the detection of gravitational waves under non-Gaussian noises II. Independent Component Analysis
• A Common Origin for Low Mass Ratio Events Observed by LIGO and Virgo in the First Half of the Third Observing Run
• Efficient method for measuring the parameters encoded in a gravitational-wave signal
• Semianalytical Approach for Sky Localization of Gravitational Waves
• Formation of the First Two Black Hole-Neutron Star Mergers (GW200115 and GW200105) from Isolated Binary Evolution
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Characterization of gravitational-wave detector noise with fractals
• Prospects for Time-Domain and Multi-Messenger Science with eXTP
• Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?
• Determination of compressive stress in thin films using micro-machined buckled membranes
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Accelerating the standard siren method: Improved constraints on modified gravitational-wave propagation with future data
• Gravitational Wave From Axion-like Particle Inflation
• Probing the large-scale structure of the universe through gravitational-wave observations
• Study of Parametric Instability of gravitational wave detectors using silicon test masses
• Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• Radio Constraints on $r$-process Nucleosynthesis by Collapsars
• Exposing Gravitational Waves below the Quantum Shot Noise
• Predicting the motion of a high-Q pendulum subject to seismic perturbations using machine learning
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Early Advanced LIGO binary neutron-star sky localization and parameter estimation
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Optomechanical cooling with simultaneous intracavity and extracavity squeezed light
• Expediting DECam Multimessenger Counterpart Searches with Convolutional Neural Networks
• Simplified optical configuration for a sloshing-speedmeter-enhanced gravitational wave detector
• Folding Gravitational-Wave Interferometers
• Are long gamma-ray bursts progenitors to merging binary black holes?
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Identifying multichannel coherent couplings and causal relationships in gravitational wave detectors
• A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
• Systematic Bias Due to Nonspinning Template Waveforms in the Gravitational Wave Parameter Estimation for Aligned-Spin Binary Black Holes
• Phase decomposition of the template metric for continuous gravitational-wave searches
• Gravitational Wave Searches with Pulsar Timing Arrays. I: Cancellation of Clock and Ephemeris Noises
• Scattering Loss in Precision Metrology due to Mirror Roughness
• Broadband Coherent Multidimensional Variational Measurement
• Design and experimental demonstration of a laser modulation system for future gravitational-wave detectors
• What to expect: kilonova light curve predictions via equation of state marginalization
• Study of selected mild steels for application in vacuum systems of future gravitational wave detectors
• Parametric Oscillatory Instability in a Fabry-Perot Cavity of the Einstein Telescope with different mirror's materials
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• A targeted spectral interpolation algorithm for the detection of continuous gravitational waves
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• Global Stellar Budget for LIGO Black Holes
• Thermal noise of beam splitters in laser gravitational wave detectors
• Quantum Bayesian Inference with Renormalization for Gravitational Waves
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Deep insights into the local structure of amorphous Ta2O5 thin films by X-ray pair distribution function analysis
• High Dynamic Range Spatial Mode Decomposition
• All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• An analytic approach for the study of pulsar spindown
• Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
• Constraining black-hole horizon effects by LIGO-Virgo detections of inspiralling binary black holes
• Nonlinear mode-tide coupling in coalescing binary neutron stars with relativistic corrections
• Displacement-noise-free interferometeric gravitational-wave detector using unidirectional neutrons with four speeds
• Reanalysis of LIGO black-hole coalescences with alternative prior assumptions
• Co-interacting dark matter and conformally coupled light scalars
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Multimessenger Probes of High-energy Sources
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Gravitational Wave Strain and Orbital Dynamics of Binary Pulsars from LIGO-Virgo to LISA
• Chirp mass based glitch identification in long duration gravitational wave transients
• Measuring nonclasicality of single-mode systems
• Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin
• Efficient Estimation of Barycentered Relative Time Delays for Distant Gravitational Wave Sources
• Fast response electromagnetic follow-ups from low latency GW triggers
• Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
• Expect the unexpected: augmented mixture models for black-hole-population studies
• Constraining Electromagnetic Signals from Black Holes with Hair
• Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical symmetry
• Enhanced optomechanical interaction in the unbalanced interferometer
• Gravitational wave and dark matter from Axion-Higgs string
• Modeling of optical scattering from topographic surface measurements of high-quality mirrors
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Evidence of large recoil velocity from a black hole merger signal
• Kilonova and progenitor properties of merger-driven gamma-ray bursts
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
• Constant-roll inflation and primordial black holes within Barrow entropic framework
• Numerical simulations of oscillating and differentially rotating neutron stars
• Quantum interference between distant creation processes
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• Gravitational-wave matched filtering on a quantum computer
• Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Reflections on "Can AI Understand Our Universe?"
• The Classical Harmonic Vibrations of the Atomic Centers of Mass with Micro Amplitudes and Low Frequencies Monitored by the Entanglement between the Two Two-level Atoms in a Single mode Cavity
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Low-Frequency Noise Mitigation and Bandgap Engineering using Seismic Metamaterials for Terrestrial Gravitational Wave Observatories
• Optimizing signal recycling for detecting a stochastic gravitational-wave background
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• Gravitational wave optical counterpart searching based on GRAWITA and DLT40 project during LIGO O2 run
• Gravitational Waves by Perturbation of a Slowly Rotating Thin-Shell Wormhole
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Operating Gravitational Wave Detectors far from equilibrium
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Gravitational-wave standard sirens and application in cosmology
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• On the ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
• Finding Fast Transients in Real Time Using Novel Light Curve Analysis Algorithm
• Gravitational-wave asteroseismology with f-modes from neutron star binaries at the merger phase
• Very-High-Frequency Gravitational Waves from Multi-Monodromy Inflation
• A machine learning algorithm for minute-long Burst searches
• Testing Nambu-Goto approximation of cosmic string by lattice field simulations
• A DESGW Search for the Electromagnetic Counterpart to the LIGO/Virgo Gravitational Wave Binary Neutron Star Merger Candidate S190510g
• Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals
• Wave-particle duality in the measurement of gravitational radiation
• Discrimination of metric theories
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits
• Comparing Bayes factors and hierarchical inference for testing general relativity with gravitational waves
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors
• Analysis and Mitigation of Crosstalk in a Multi-Parameter Laser Beam Diagnostic System
• Distinguishing between dark-matter interactions with gravitational-wave detectors
• Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations
• Probing High Scale Dirac Leptogenesis via Gravitational Waves from Domain Walls
• Analysing one- and two-bit data to reduce memory requirements for F-statistic-based gravitational wave searches