Identification of Binary Neutron Star Mergers in Gravitational-Wave Data
Using YOLO One-Shot Object Detection
- URL: http://arxiv.org/abs/2207.00591v1
- Date: Fri, 1 Jul 2022 10:11:44 GMT
- Title: Identification of Binary Neutron Star Mergers in Gravitational-Wave Data
Using YOLO One-Shot Object Detection
- Authors: Jo\~ao Aveiro, Felipe F. Freitas, M\'arcio Ferreira, Antonio Onofre,
Constan\c{c}a Provid\^encia, Gon\c{c}alo Gon\c{c}alves, and Jos\'e A. Font
- Abstract summary: We demonstrate the application of the YOLOv5 model, a general purpose convolution-based single-shot object detection model, in the task of detecting binary neutron star (BNS) coalescence events from gravitational-wave data of current generation interferometer detectors.
We achieve mean average precision ($textmAP_[0.50]$) values of 0.945 for a single class validation dataset and as high as 0.978 for test datasets.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: We demonstrate the application of the YOLOv5 model, a general purpose
convolution-based single-shot object detection model, in the task of detecting
binary neutron star (BNS) coalescence events from gravitational-wave data of
current generation interferometer detectors. We also present a thorough
explanation of the synthetic data generation and preparation tasks based on
approximant waveform models used for the model training, validation and testing
steps. Using this approach, we achieve mean average precision
($\text{mAP}_{[0.50]}$) values of 0.945 for a single class validation dataset
and as high as 0.978 for test datasets. Moreover, the trained model is
successful in identifying the GW170817 event in the LIGO H1 detector data. The
identification of this event is also possible for the LIGO L1 detector data
with an additional pre-processing step, without the need of removing the large
glitch in the final stages of the inspiral. The detection of the GW190425 event
is less successful, which attests to performance degradation with the
signal-to-noise ratio. Our study indicates that the YOLOv5 model is an
interesting approach for first-stage detection alarm pipelines and, when
integrated in more complex pipelines, for real-time inference of physical
source parameters.
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