Gwbench: a novel Fisher information package for gravitational-wave benchmarking
arXiv:2010.15202 · doi:10.1088/1361-6382/ac1618
Abstract
We present a new Python package, gwbench, implementing the well-established Fisher information formalism as a fast and straightforward tool for the purpose of gravitational-wave benchmarking, i.e. the estimation of signal-to-noise ratios and measurement errors of gravitational waves observed by a network of detectors. Such an infrastructure is necessary due to the high computational cost of Bayesian parameter estimation methods which renders them less effective for the scientific assessment of gravitational waveforms, detectors, and networks of detectors, especially when determining their effects on large populations of gravitational-wave sources spread throughout the universe. gwbench further gives quick access to detector locations and sensitivities, while including the effects of Earth's rotation on the latter, as well as waveform models and their derivatives, while giving access to the host of waveforms available in the LSC Algorithm Library. With the provided functionality, gwbench is relevant for a wide variety of applications in gravitational-wave astronomy such as waveform modeling, detector development, cosmology, and tests of general relativity.
arXiv comment18 pages, 6 figures, 4 tables
References in corpus (45)
- Astropy: A Community Python Package for Astronomy
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Advanced LIGO
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- GW190521: A Binary Black Hole Merger with a Total Mass of
- Science Case for the Einstein Telescope
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Interferometer design of the KAGRA gravitational wave detector
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
- Black holes, gravitational waves and fundamental physics: a roadmap
- Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Search templates for gravitational waves from inspiraling binaries: Choice of template spacing
- Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
- Matched filtering of gravitational waves from inspiraling compact binaries: Computational cost and template placement
- Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
- Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms
- Networks of gravitational wave detectors and three figures of merit
- Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
- Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
- Gravitational waves from inspiraling compact binaries: The quadrupole-moment term
- First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
- Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars
- A Cryogenic Silicon Interferometer for Gravitational-wave Detection
- Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
- Gravitational-wave parameter estimation with autoregressive neural network flows
- Next-to-next-to-leading order spin-orbit effects in the gravitational wave flux and orbital phasing of compact binaries
- Probing the non-linear structure of general relativity with black hole binaries
- PyCBC Live: Rapid Detection of Gravitational Waves from Compact Binary Mergers
- Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
- Self-interaction spin effects in inspiralling compact binaries
- Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
- Learning Bayesian posteriors with neural networks for gravitational-wave inference
- Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
- Are stellar-mass black-hole binaries too quiet for LISA?
- Dark Sirens to Resolve the Hubble-Lemaître Tension
- SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries
- Multiparameter tests of general relativity using multiband gravitational-wave observations
- Verifying the no-hair property of massive compact objects with intermediate-mass-ratio inspirals in advanced gravitational-wave detectors
Cited by in corpus (69)
- Science with the Einstein Telescope: a comparison of different designs
- Forecasting the detection capabilities of third-generation gravitational-wave detectors using
- The Science of the Einstein Telescope
- : a Fisher information matrix Python code for third-generation gravitational-wave detectors
- GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
- Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
- Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
- Constraints on the maximum densities of neutron stars from postmerger gravitational waves with third-generation observations
- Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
- Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
- Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
- Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
- Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
- Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
- Cosmography with next-generation gravitational wave detectors
- Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
- Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
- Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors
- Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
- Neutron star-black hole mergers in next generation gravitational-wave observatories
- Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
- Source Confusion from Neutron Star Binaries in Ground-Based Gravitational Wave Detectors is Minimal
- Using Gray Sirens to Resolve the Hubble-Lemaître Tension
- Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
- Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors
- Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
- Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs
- Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
- Constraining extended cosmologies with GWLSS cross-correlations
- Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
- The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors
- Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
- Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
- Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
- Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
- Validating Prior-informed Fisher-matrix Analyses against GWTC Data
- GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
- Detectability of gravitational higher order modes in the third-generation era
- Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
- Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
- Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
- The Critical Role of LIGO-India in the Era of Next-Generation Observatories
- Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
- Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
- Probing dark matter halo profiles with multi-band observations of gravitational waves
- Inferring three-nucleon couplings from multi-messenger neutron-star observations
- Forecasting the population properties of merging black holes
- Multiparameter multipolar test of general relativity with gravitational waves
- Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
- Inferring small neutron star spins with neutron star-black hole mergers
- Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
- A Fisher matrix for gravitational-wave population inference
- Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars
- Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
- Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
- Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna
- Potential impact of noise correlation in next-generation gravitational wave detectors
- Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
- How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
- Impact of Population III stars on the astrophysical gravitational-wave background
- Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
- Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe
- Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
- Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
- Adding Gamma-ray Polarimetry to the Multi-Messenger Era
- Primordial black holes versus their impersonators at gravitational wave observatories
- Impact of facility timing and coordination for next-generation gravitational-wave detectors
- Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
- Golden and Silver Dark Sirens for precise H0 measurement with HETDEX