A Neural Network Approach to Preferred Event Selection for Low-Latency Gravitational-Wave Alerts

arXiv:2511.14997 · astro-ph.IM, astro-ph.HE, gr-qc · Submitted 2025-11-19 · Read on arXiv

astro-ph.IM, astro-ph.HE, gr-qc

Submitted: 2025-11-19

Updated: 2026-09-22

Terminology

• Accuracy — 3× in this paper · explained in 1 episode
• Adam — 3× in this paper · explained in 2 episodes
• Generalization — 3× in this paper · explained in 13 episodes
• Regularization — 3× in this paper · explained in 3 episodes
• Robustness — 3× in this paper · explained in 5 episodes
• Adaptation — 2× in this paper · explained in 1 episode
• Loss Function — 2× in this paper · explained in 2 episodes
• Signal-to-noise ratio (SNR) — 2× in this paper · explained in 2 episodes
• Activation Function — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Covariate Shift — 1× in this paper · explained in 2 episodes
• Gradient Flow — 1× in this paper · explained in 2 episodes
• Objective Function — 1× in this paper · explained in 2 episodes
• Redundancy — 1× in this paper · explained in 2 episodes

Sources

• Advanced LIGO
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Overview of KAGRA: Detector design and construction history
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Localization and broadband follow-up of the gravitational-wave transient GW150914
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Observation of gravitational waves from two neutron star-black hole coalescences
• An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
• INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• A kilonova as the electromagnetic counterpart to a gravitational-wave source
• Multi-messenger Observations of a Binary Neutron Star Merger
• Neutron-star radius constraints from GW170817 and future detections
• Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
• Multi-messenger Bayesian parameter inference of a binary neutron-star merger
• Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations
• Implications of the search for optical counterparts during the first six months of the Advanced LIGO's and Advanced Virgo's third observing run: possible limits on the ejecta mass and binary properties
• Gravitational-wave constraints on the neutron-star-matter Equation of State
• GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations

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