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Analysis

This paper introduces LUNCH, a deep-learning framework designed for real-time classification of high-energy astronomical transients. The significance lies in its ability to classify transients directly from raw light curves, bypassing the need for traditional feature extraction and localization. This is crucial for timely multi-messenger follow-up observations. The framework's high accuracy, low computational cost, and instrument-agnostic design make it a practical solution for future time-domain missions.
Reference

The optimal model achieves 97.23% accuracy when trained on complete energy spectra.