Summed Parallel Infinite Impulse Response (SPIIR) Filters For Low-Latency Gravitational Wave Detection
arXiv:1108.3186 · doi:10.1103/PhysRevD.86.024012
Abstract
With the upgrade of current gravitational wave detectors, the first detection of gravitational wave signals is expected to occur in the next decade. Low-latency gravitational wave triggers will be necessary to make fast follow-up electromagnetic observations of events related to their source, e.g., prompt optical emission associated with short gamma-ray bursts. In this paper we present a new time-domain low-latency algorithm for identifying the presence of gravitational waves produced by compact binary coalescence events in noisy detector data. Our method calculates the signal to noise ratio from the summation of a bank of parallel infinite impulse response (IIR) filters. We show that our summed parallel infinite impulse response (SPIIR) method can retrieve the signal to noise ratio to greater than 99% of that produced from the optimal matched filter. We emphasise the benefits of the SPIIR method for advanced detectors, which will require larger template banks.
9 pages, 6 figures, for PRD
References in corpus (6)
- Gamma-Ray Bursts: Progress, Problems & Prospects
- Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
- Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data
- Singular value decomposition applied to compact binary coalescence gravitational-wave signals
- Towards low-latency real-time detection of gravitational waves from compact binary coalescences in the era of advanced detectors
- Interpreting the results of searches for gravitational waves from coalescing binaries
Cited by in corpus (53)
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- GW190521: A Binary Black Hole Merger with a Total Mass of
- Observation of gravitational waves from two neutron star-black hole coalescences
- PyCBC Live: Rapid Detection of Gravitational Waves from Compact Binary Mergers
- Implications of Eccentric Observations on Binary Black Hole Formation Channels
- Extending the PyCBC search for gravitational waves from compact binary mergers to a global network
- Realtime search for compact binary mergers in Advanced LIGO and Virgo's third observing run using PyCBC Live
- Detection of gravitational-wave signals from binary neutron star mergers using machine learning
- First demonstration of early warning gravitational wave alerts
- Capturing the electromagnetic counterparts of binary neutron star mergers through low latency gravitational wave triggers
- A Machine Learning Based Source Property Inference for Compact Binary Mergers
- Training Strategies for Deep Learning Gravitational-Wave Searches
- Gravitational-wave inference in the catalog era: evolving priors and marginal events
- Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
- Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
- A Search for Gravitational Waves from Binary Mergers with a Single Observatory
- Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
- Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
- Using negative-latency gravitational wave alerts to detect prompt radio bursts from binary neutron star mergers with the Murchison Widefield Array
- Early Warnings of Binary Neutron Star Coalescence using the SPIIR Search
- Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
- Gravitational wave detection without boot straps: a Bayesian approach
- Establishing significance of gravitational-wave signals from a single observatory in the PyCBC offline search
- Predicting electromagnetic counterparts using low-latency, gravitational-wave data products
- Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
- Hierarchical approach to matched filtering using a reduced basis
- Search for Advanced LIGO Single Interferometer Compact Binary Coalescence Signals in Coincidence with Gamma-Ray Events in Fermi-GBM
- The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
- Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
- Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
- Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
- The SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences
- Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
- Bayesian Inference Analysis of Unmodelled Gravitational-Wave Transients
- Gravitational wave astrophysics, data analysis and multimessenger astronomy
- Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role
- Quasi-periodic oscillation in short gamma-ray bursts from black hole-neutron star mergers
- Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
- Blind source separation in 3rd generation gravitational-wave detectors
- Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
- Semianalytical Approach for Sky Localization of Gravitational Waves
- The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
- Gravitational-wave searches in the era of Advanced LIGO and Virgo
- The constraint ability of Hubble parameter by gravitational wave standard sirens on cosmological parameters
- What to expect: kilonova light curve predictions via equation of state marginalization
- Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
- Fast response electromagnetic follow-ups from low latency GW triggers
- Sky localization of gravitational waves from eccentric binaries
- Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
- Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
- Enhancing online estimation of CBC parameters with the low-latency MBTA analysis