Detection and Parameter Estimation of Gravitational Waves from Binary Neutron-Star Mergers in Real LIGO Data using Deep Learning. (arXiv:2012.13101v2 [astro-ph.IM] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Krastev_P/0/1/0/all/0/1">Plamen G. Krastev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gill_K/0/1/0/all/0/1">Kiranjyot Gill</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Villar_V/0/1/0/all/0/1">V. Ashley Villar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Berger_E/0/1/0/all/0/1">Edo Berger</a>
One of the key challenges of real-time detection and parameter estimation of
gravitational waves from compact binary mergers is the computational cost of
conventional matched-filtering and Bayesian inference approaches. In
particular, the application of these methods to the full signal parameter space
available to the gravitational-wave detectors, and/or real-time parameter
estimation is computationally prohibitive. On the other hand, rapid detection
and inference are critical for prompt follow-up of the electromagnetic and
astro-particle counterparts accompanying important transients, such as binary
neutron-star and black-hole neutron-star mergers. Training deep neural networks
to identify specific signals and learn a computationally efficient
representation of the mapping between gravitational-wave signals and their
parameters allows both detection and inference to be done quickly and reliably,
with high sensitivity and accuracy. In this work we apply a deep-learning
approach to rapidly identify and characterize transient gravitational-wave
signals from binary neutron-star mergers in real LIGO data. We show for the
first time that artificial neural networks can promptly detect and characterize
binary neutron star gravitational-wave signals in real LIGO data, and
distinguish them from noise and signals from coalescing black-hole binaries. We
illustrate this key result by demonstrating that our deep-learning framework
classifies correctly all gravitational-wave events from the Gravitational-Wave
Transient Catalog, GWTC-1 [Phys. Rev. X 9 (2019), 031040]. These results
emphasize the importance of using realistic gravitational-wave detector data in
machine learning approaches, and represent a step towards achieving real-time
detection and inference of gravitational waves.
One of the key challenges of real-time detection and parameter estimation of
gravitational waves from compact binary mergers is the computational cost of
conventional matched-filtering and Bayesian inference approaches. In
particular, the application of these methods to the full signal parameter space
available to the gravitational-wave detectors, and/or real-time parameter
estimation is computationally prohibitive. On the other hand, rapid detection
and inference are critical for prompt follow-up of the electromagnetic and
astro-particle counterparts accompanying important transients, such as binary
neutron-star and black-hole neutron-star mergers. Training deep neural networks
to identify specific signals and learn a computationally efficient
representation of the mapping between gravitational-wave signals and their
parameters allows both detection and inference to be done quickly and reliably,
with high sensitivity and accuracy. In this work we apply a deep-learning
approach to rapidly identify and characterize transient gravitational-wave
signals from binary neutron-star mergers in real LIGO data. We show for the
first time that artificial neural networks can promptly detect and characterize
binary neutron star gravitational-wave signals in real LIGO data, and
distinguish them from noise and signals from coalescing black-hole binaries. We
illustrate this key result by demonstrating that our deep-learning framework
classifies correctly all gravitational-wave events from the Gravitational-Wave
Transient Catalog, GWTC-1 [Phys. Rev. X 9 (2019), 031040]. These results
emphasize the importance of using realistic gravitational-wave detector data in
machine learning approaches, and represent a step towards achieving real-time
detection and inference of gravitational waves.
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