Rapid and Robust Parameter Inference for Binary Mergers
arXiv:2101.01188 · doi:10.1103/PhysRevD.103.104057
Abstract
The detection rate for compact binary mergers has grown as the sensitivity of the global network of ground based gravitational wave detectors has improved, now reaching the stage where robust automation of the analyses is essential. Automated low-latency algorithms have been developed that send out alerts when candidate signals are detected. The alerts include sky maps to facilitate electromagnetic follow up observations, along with probabilities that the system might contain a neutron star, and hence be more likely to generate an electromagnetic counterpart. Data quality issues, such as loud noise transients (glitches), can adversely affect the low-latency algorithms, causing false alarms and throwing off parameter estimation. Here a new analysis method is presented that is robust against glitches, and capable of producing fully Bayesian parameter inference, including sky maps and mass estimates, in a matter of minutes. Key elements of the method are wavelet-based de-noising, penalized maximization of the likelihood during the initial search, rapid sky localization using pre-computed inner products, and heterodyned likelihoods for full Bayesian inference.
arXiv comment13 pages, 11 figures
References in corpus (36)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Binary Black Hole Mergers in the first Advanced LIGO Observing Run
- Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
- A simple model of complete precessing black-hole-binary gravitational waveforms
- The PyCBC search for gravitational waves from compact binary coalescence
- Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
- BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
- Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
- Rapid Bayesian position reconstruction for gravitational-wave transients
- A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
- A chi-squared time-frequency discriminator for gravitational wave detection
- Deep Learning for Real-time Gravitational Wave Detection and Parameter Estimation: Results with Advanced LIGO Data
- Dynamic temperature selection for parallel-tempering in Markov chain Monte Carlo simulations
- BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
- First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
- Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects
- Massively parallel Bayesian inference for transient gravitational-wave astronomy
- Low-latency analysis pipeline for compact binary coalescences in the advanced gravitational wave detector era
- The BayesWave analysis pipeline in the era of gravitational wave observations
- Effects of Data Quality Vetoes on a Search for Compact Binary Coalescences in Advanced LIGO's First Observing Run
- A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
- Machine-learning non-stationary noise out of gravitational wave detectors
- Improving the Sensitivity of Advanced LIGO Using Noise Subtraction
- Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
- Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO
- Realtime search for compact binary mergers in Advanced LIGO and Virgo's third observing run using PyCBC Live
- Reconstructing the calibrated strain signal in the Advanced LIGO detectors
- A Bayesian Approach to the Detection Problem in Gravitational Wave Astronomy
- Accelerating parameter inference with graphics processing units
- Modeling compact binary signals and instrumental glitches in gravitational wave data
- Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
- Black Hole Hunting with LISA
Cited by in corpus (22)
- Real-time gravitational-wave science with neural posterior estimation
- Parameter estimation with gravitational waves
- Heterodyned Likelihood for Rapid Gravitational Wave Parameter Inference
- Accelerating parameter estimation of gravitational waves from compact binary coalescence using adaptive frequency resolutions
- Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
- Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
- Transient glitch mitigation in Advanced LIGO data with
- The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
- Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
- Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
- Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
- Low Latency Detection of Massive Black Hole Binaries
- Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
- Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
- Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
- Semianalytical Approach for Sky Localization of Gravitational Waves
- Inferring Binary Properties from Gravitational Wave Signals
- Optimized localization for gravitational-waves from merging binaries
- Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
- labrador: A domain-optimized machine-learning tool for gravitational wave inference
- Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
- MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data