Classification of Transient Astronomical Object Light Curves Using LSTM Neural Networks
Guilherme Grancho D. Fernandes, Marco A. Barroca, Mateus dos Santos, Rafael S. Oliveira

TL;DR
This paper develops a bidirectional LSTM neural network to classify transient astronomical objects from light curves, achieving high accuracy for some classes but struggling with others, especially under limited data conditions.
Contribution
Introduces a novel LSTM-based approach with class reorganization and preprocessing to improve transient object classification from astronomical light curves.
Findings
High ROC AUC for S-Like (0.95) and Periodic (0.99) classes.
Lower performance for Fast and Long classes (ROC AUC 0.68).
Performance drops with shorter observation windows.
Abstract
This study presents a bidirectional Long Short-Term Memory (LSTM) neural network for classifying transient astronomical object light curves from the Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC) dataset. The original fourteen object classes were reorganized into five generalized categories (S-Like, Fast, Long, Periodic, and Non-Periodic) to address class imbalance. After preprocessing with padding, temporal rescaling, and flux normalization, a bidirectional LSTM network with masking layers was trained and evaluated on a test set of 19,920 objects. The model achieved strong performance for S-Like and Periodic classes, with ROC area under the curve (AUC) values of 0.95 and 0.99, and Precision-Recall AUC values of 0.98 and 0.89, respectively. However, performance was significantly lower for Fast and Long classes (ROC AUC of 0.68 for Long class), and the…
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Taxonomy
TopicsTime Series Analysis and Forecasting · Astronomical Observations and Instrumentation · Stellar, planetary, and galactic studies
