The reviewed record of science sign in
Pith

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

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

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 kernel pith:RM5QTM6Jrecord.jsonopen to challenge →

classification astro-ph.IM
keywords uncertaintyastronomicalestimationevaluatedlightthreeabilityallowing
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.