Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
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- Type
- article
- Published
- 2018-05-16
- Cited by
- 103
- References
- 116
- Access
- Open access
- OpenAlex
- https://openalex.org/W2803232194
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:119061163
Keywords
LIGO, Physics, Gravitational wave, Context (archaeology), Population
References
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- Nonspinning searches for spinning binaries in ground-based detector data: Amplitude and mismatch predictions in the constant precession cone approximation
- Intrinsic selection biases of ground-based gravitational wave searches for high-mass black hole-black hole mergers
- Parameter estimation of gravitational waves from nonprecessing black hole-neutron star inspirals with higher harmonics: Comparing Markov-chain Monte Carlo posteriors to an effective Fisher matrix
- Methods of information geometry
- Accounting for Source Uncertainties in Analyses of Astronomical Survey Data
- Simple model of complete precessing black-hole-binary gravitational waveforms.
- DOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES
- I and i
- Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars
- OBSCURATION-DEPENDENT EVOLUTION OF ACTIVE GALACTIC NUCLEI
- Systematic parameter errors in inspiraling neutron star binaries.
- Compact binary coalescences in the band of ground-based gravitational-wave detectors
- DOUBLE COMPACT OBJECTS. I. THE SIGNIFICANCE OF THE COMMON ENVELOPE ON MERGER RATES
- Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
- Pair-Instability Supernovae, Gravity Waves, and Gamma-Ray Transients
- Gravitational waves from inspiraling compact binaries: Parameter estimation using second-post-Newtonian waveforms.
- Advanced Virgo: a second-generation interferometric gravitational wave detector
- Avoiding selection bias in gravitational wave astronomy
- Application of the effective Fisher matrix to the frequency domain inspiral waveforms
Cited by
- Rapid and accurate parameter inference for coalescing, precessing compact binaries
- Does the Black Hole Merger Rate Evolve with Redshift?
- The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
- Constraints on binary black hole populations from LIGO–Virgo detections
- An introduction to Bayesian inference in gravitational-wave astronomy: Parameter estimation, model selection, and hierarchical models
- Constraining Black Hole Spins with Gravitational-wave Observations
- Extracting distribution parameters from multiple uncertain observations with selection biases
- Astrophysics of stellar black holes
- Stochastic Gravitational-wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
- A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model
- Distinguishing primordial black holes from astrophysical black holes by Einstein Telescope and Cosmic Explorer
- The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution
- Higher order gravitational-wave modes with likelihood reweighting
- Unraveling the origin of black holes from effective spin measurements with LIGO-Virgo
- Monte Carlo simulations of black hole mergers in AGN discs: Low χeff mergers and predictions for LIGO
- When will we observe binary black holes precessing?
- Label switching problem in Bayesian analysis for gravitational wave astronomy
- Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
- Two-harmonic approximation for gravitational waveforms from precessing binaries
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
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