GSpyNetTree: a signal-vs-glitch classifier for gravitational-wave event candidates

S. Álvarez-López, Annudesh Liyanage, Julian Ding, Raymond T. Ng, J. McIver

Classical and Quantum Gravity 2024 article cited by 14

importance 6/10 ai assisted Pulsars and Gravitational Waves Research gravitational-wave astronomy stage: research

LIGO-Virgo detector data contain non-Gaussian transient noise 'glitches' that can mimic real gravitational-wave signals, and the higher expected O4 event rate requires automated candidate validation.

Glitches that mimic signals can cause false or missed gravitational-wave detections, undermining astrophysical discoveries.

Restructures the Gravity Spy machine learning tool into GSpyNetTree, a compact binary coalescence signal-vs-glitch classifier to distinguish glitches from real GW signals.

not stated in source

The classifier addresses automation needs for O4 candidate validation; performance figures not stated in source.

Venue Classical and Quantum Gravity
Published 2024
Work type article
Authors S. Álvarez-López, Annudesh Liyanage, Julian Ding, Raymond T. Ng, J. McIver
Citations 14 (OpenAlex, at import time)
References 66
Model or method GSpyNetTree (Gravity Spy-based machine learning)
Organization LIGO-Virgo (detectors referenced in abstract)
Primary source https://doi.org/10.1088/1361-6382/ad2194
Open access hybrid
Keywords gravitational waves, glitches, machine learning, LIGO, classifier, signal detection
6 / 10

significant — thousands to millions affected

Glitches frequently mimic real GW signals and higher expected O4 event rate requires automated validation; affects astrophysical discovery in a foundational field, scale not quantified.

Basis: inferred. Judged from the source text, which gives no explicit scale. Stated scale: not stated in source. Method and limits.

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