Estimation of parameters of gravitational waves from coalescing binaries
arXiv:gr-qc/9708003 · doi:10.1103/PhysRevD.57.3408
Abstract
The paper deals with the estimation of parameters of gravitational waves from coalescing binaries. It explains the discrepancy between the Monte carlo simulations and the covariance matrix. We include the post-Newtonian as well as the Newtonian case.
Revtex file with figures included(18)
Cited by in corpus (24)
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Measuring gravitational waves from binary black hole coalescences: II. the waves' information and its extraction, with and without templates
- Gravitational waves from inspiraling compact binaries: The quadrupole-moment term
- Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
- Gravitational waves from inspiraling compact binaries: Validity of the stationary-phase approximation to the Fourier transform
- Testing the binary black hole nature of a compact binary coalescence
- Measuring the parameters of massive black hole binary systems with Pulsar Timing Array observations of gravitational waves
- Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries
- Testing General Relativity using Bayesian model selection: Applications to observations of gravitational waves from compact binary systems
- Gravitational-Wave Data Analysis. Formalism and Sample Applications: The Gaussian Case
- Parameter estimation for Galactic binaries by LISA
- Estimating the parameters of non-spinning binary black holes using ground-based gravitational-wave detectors: Statistical errors
- Binary black hole spectroscopy
- Gravitational waves from eccentric compact binaries: Reduction in signal-to-noise ratio due to nonoptimal signal processing
- Detection of gravitational wave bursts by interferometric detectors
- Beyond Fisher: exact sampling distributions of the maximum-likelihood estimator in gravitational-wave parameter estimation
- Gravitational waves from inspiralling compact binaries with magnetic dipole moments
- Detection and Parameter Estimation of Gravitational Waves from Compact Binary Inspirals with Analytical Double-Precessing Templates
- Generic bounds on dipolar gravitational radiation from inspiralling compact binaries
- Parameter estimation from Gravitational waves generated by non-spinning binary black holes with laser interferometers: beyond the Fisher information
- Application of asymptotic expansions of maximum likelihood estimators errors to gravitational waves from binary mergers: the single interferometer case
- Detecting gravitational waves from inspiraling binaries with a network of detectors : coherent versus coincident strategies
- Detecting gravitational waves from inspiraling binaries with a network of geographically separated detectors: coherent versus coincident strategies