SELDON: Supernova Explosions Learned by Deep ODE Networks
Jiezhong Wu, Jack O'Brien, Jennifer Li, M. S. Krafczyk, Ved G. Shah, Amanda R. Wasserman, Daniel W. Apley, Gautham Narayan, Noelle I. Samia

TL;DR
SELDON is a novel deep learning model that accurately forecasts and interprets irregular, sparse astrophysical light curves in continuous time, enabling rapid analysis of millions of transient events.
Contribution
The paper introduces SELDON, a continuous-time variational autoencoder combining neural ODEs and interpretable Gaussian basis decoding for astrophysical light curves, improving inference speed and interpretability.
Findings
Handles sparse, irregular, and nonstationary data effectively.
Provides physically meaningful parameters for astrophysical analysis.
Enables rapid, millisecond-scale inference for large datasets.
Abstract
The discovery rate of optical transients will explode to 10 million public alerts per night once the Vera C. Rubin Observatory's Legacy Survey of Space and Time comes online, overwhelming the traditional physics-based inference pipelines. A continuous-time forecasting AI model is of interest because it can deliver millisecond-scale inference for thousands of objects per day, whereas legacy MCMC codes need hours per object. In this paper, we propose SELDON, a new continuous-time variational autoencoder for panels of sparse and irregularly time-sampled (gappy) astrophysical light curves that are nonstationary, heteroscedastic, and inherently dependent. SELDON combines a masked GRU-ODE encoder with a latent neural ODE propagator and an interpretable Gaussian-basis decoder. The encoder learns to summarize panels of imbalanced and correlated data even when only a handful of points are…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Gaussian Processes and Bayesian Inference · Galaxies: Formation, Evolution, Phenomena
