SIGNN – Star Identification Using Graph Neural Networks

As a solution for the lost-in-space star identification problem we present Star Identification using Graph Neural Network (SIGNN), a novel approach using Graph Attention Networks. By representing the celestial sphere as a graph data structure, created from the ESA's Hipparcos catalogue, we are able to accurately capture the rich information and relationships within local star fields. Graph learning techniques allow our model to aggregate information and learn the relative importance of the nodes and structure within each stars local neighbourhood to it's identification. This approach, combined with our parametric data-generation and noise simulation, allows us to train a highly robust model capable of accurate star identification even under intensive noise, outperforming existing methods. Code and generation techniques will be available on https://github.com/FloydHepburn/SIGNN.

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Publication Details

Published
2025-02-26
DOI
https://doi.org/10.1109/wacv61041.2025.00878
Citations
2
Primary Topic
Astronomical Observations and Instrumentation
Type
article
Field-Weighted Citation Impact
2.67
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article

SIGNN – Star Identification Using Graph Neural Networks

Mark W. Jones, Steve Bell, Michael Edwards, Floyd Hepburn-Dickins et al.
2 citations
Astronomical Observations and Instrumentation
2.67
article

SIGNN – Star Identification Using Graph Neural Networks

Mark W. Jones, Steve Bell, Michael Edwards, Floyd Hepburn-Dickins, Jay Morgan
article en
2 citations

Abstract

As a solution for the lost-in-space star identification problem we present Star Identification using Graph Neural Network (SIGNN), a novel approach using Graph Attention Networks. By representing the celestial sphere as a graph data structure, created from the ESA's Hipparcos catalogue, we are able to accurately capture the rich information and relationships within local star fields. Graph learning techniques allow our model to aggregate information and learn the relative importance of the nodes and structure within each stars local neighbourhood to it's identification. This approach, combined with our parametric data-generation and noise simulation, allows us to train a highly robust model capable of accurate star identification even under intensive noise, outperforming existing methods. Code and generation techniques will be available on https://github.com/FloydHepburn/SIGNN.

Swansea University (GB), Taunton & Somerset NHS Foundation Trust (GB)
Openalex Percentile: Top 13%
Astronomical Observations and Instrumentation
2.67
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