Towards a unified treatment of gravitational-wave data analysis
arXiv:1305.2934 · doi:10.1103/PhysRevD.87.122003
Abstract
We present a unified description of gravitational-wave data analysis that unites the template-based analysis used to detect deterministic signals from well-modeled sources, such as binary-black-hole mergers, with the cross-correlation analysis used to detect stochastic gravitational-wave backgrounds. We also discuss the connection between template-based analyses and those that target poorly-modeled bursts of gravitational waves, and suggest a new approach for detecting burst signals.
4 pages, no figures, published version
References in corpus (5)
- Coherent network analysis technique for discriminating gravitational-wave bursts from instrumental noise
- Long gravitational-wave transients and associated detection strategies for a network of terrestrial interferometers
- Detection methods for non-Gaussian gravitational wave stochastic backgrounds
- Search method for long-duration gravitational-wave transients from neutron stars
- The cross-correlation search for periodic gravitational waves
Cited by in corpus (18)
- Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
- BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
- Detecting dark matter waves with precision measurement tools
- Mapping gravitational-wave backgrounds using methods from CMB analysis: Application to pulsar timing arrays
- The Science of the Einstein Telescope
- Pulsar Timing Array Analysis for Black Hole Backgrounds
- Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
- Searching for gravitational-wave transients with a qualitative signal model: seedless clustering strategies
- Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
- Cross-correlation method for intermediate-duration gravitational wave searches associated with gamma-ray bursts
- When is a gravitational-wave signal stochastic?
- Probing Stochastic Ultralight Dark Matter with Space-based Gravitational-Wave Interferometers
- Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
- Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
- Handling Data Gaps for the Next Generation of Gravitational-Wave Observatories
- Rapid inference for individual binaries and a stochastic background with pulsar timing array data
- Cross-Spectrum Measurement Statistics
- Fast Bayesian analysis of individual binaries in pulsar timing array data