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Transformer-Based Astronomical Time Series Model with Uncertainty Estimation for Detecting Misclassified Instances

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arxiv 2411.01363 v1 pith:RM5QTM6J submitted 2024-11-02 astro-ph.IM

classification astro-ph.IM
keywords uncertaintyastronomicalestimationevaluatedlightthreeabilityallowing
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In this work, we present a framework for estimating and evaluating uncertainty in deep-attention-based classifiers for light curves for variable stars. We implemented three techniques, Deep Ensembles (DEs), Monte Carlo Dropout (MCD) and Hierarchical Stochastic Attention (HSA) and evaluated models trained on three astronomical surveys. Our results demonstrate that MCD and HSA offers a competitive and computationally less expensive alternative to DE, allowing the training of transformers with the ability to estimate uncertainties for large-scale light curve datasets. We conclude that the quality of the uncertainty estimation is evaluated using the ROC AUC metric.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Image-Based Multi-Survey Classification of Light Curves with a Pre-Trained Vision Transformer

    astro-ph.IM 2025-07 conditional novelty 5.0 of 10

    A shared-weights two-branch Swin Transformer that processes ZTF and ATLAS light curves jointly reaches 69.9% macro F1, outperforming single-survey models and simple fusion strategies on 21 classes.

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