GWSkyNet: A Real-time Classifier for Public Gravitational-wave Candidates
Creators
- 1. Department of Physics and Astronomy, The University of British Columbia, Vancouver, BC V6T 1Z4 (Canada)
- 2. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States)
Description
The rapid release of accurate sky localization for gravitational-wave (GW) candidates is crucial for multi-messenger observations. During the third observing run of Advanced LIGO and Advanced Virgo, automated GW alerts were publicly released within minutes of detection. Subsequent inspection and analysis resulted in the eventual retraction of a fraction of the candidates. Updates could be delayed by up to several days, sometimes issued during or after exhaustive multi-messenger follow-up campaigns. We introduce GWSkyNet, a real-time framework to distinguish between astrophysical events and instrumental artifacts using only publicly available information from the LIGO-Virgo open public alerts. This framework consists of a non-sequential convolutional neural network involving sky maps and metadata. GWSkyNet achieves a prediction accuracy of 93.5% on a testing data set.
Availability note (English)
Available from http://dx.doi.org/10.3847/2041-8213/abc5b5Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal Letters
- Journal Volume
- 904
- Journal Issue
- 1
- Journal Page Range
- [6 p.]
- ISSN
- 2041-8205
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52056536
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCURACY; ASTROPHYSICS; DETECTION; FORECASTING; GRAVITATIONAL WAVES; NEURAL NETWORKS
- Descriptors DEC
- PHYSICS