Leveraging Multimodality for Real-Time Classification of Transients and Variables found by the Zwicky Transient Facility
Ved G. Shah, Nabeel Rehemtulla, Adam A. Miller, Sushant Sharma Chaudhary, Michael W. Coughlin, Antoine Le Calloch, Matthew J. Graham, Joahan Castaneda Jaimes, Theophile Jegou du Laz, Ashish A. Mahabal, Frank J. Masci, Josiah Purdum, Reed Riddle, Jesper Sollerman, Anastasia Wei, Mansi M. Kasliwal
astro-ph.IM, astro-ph.HE, cs.LG
Submitted: 2026-06-30
Comments: 29 Pages, 15 Figures, 8 Tables. Comments welcome
Code: https://github.com/dev-ved30/Oracle
License: http://creativecommons.org/licenses/by/4.0/
The gist: Modern time-domain surveys such as the Zwicky Transient Facility (ZTF) generate hundreds of thousands of alerts each night, making real-time decisions for follow-up observations a central challenge
Terminology
Abstract
Modern time-domain surveys such as the Zwicky Transient Facility (ZTF) generate hundreds of thousands of alerts each night, making real-time decisions for follow-up observations a central challenge in time-domain astronomy. Robust early classification is crucial for making informed decisions, but is hindered by sparse light curves and degeneracies between classes. In this work, we leverage multimodality to substantially improve real-time classification and demonstrate the practicality of our approach by deploying our model on the ZTF alert stream. Building on the Online Ranked Astrophysical CLass Estimator (ORACLE), we introduce the ORACLE-2 models, which combine light curves, metadata, and images for real-time hierarchical classification. Using both real and simulated datasets, we show that incorporating additional modalities consistently improves classification performance. On observations from ZTF's Bright Transient Survey, our best-performing model, ORACLE-2 Omni, achieves a macro F1 score of 0.73 -- an improvement of up to 11% over models using light curves and metadata alone, and up to 40% over light-curve-only models, with the strongest gains realized at early times. To demonstrate applicability to the Legacy Survey of Space and Time, which will increase alert volume by more than an order of magnitude, we train a light curve + metadata variant on the simulated ELAsTiCC dataset. This model achieves a macro F1 score of 0.88, an improvement of up to 13% over the light-curve-only variant, matching the performance of other state-of-the-art models. Finally, we quantify the trade-offs between performance and throughput, identifying regimes where multimodal approaches offer the greatest benefit. These results show that combining multiple modalities improves early-time classification, enabling more effective triage of high-volume alert streams for current and future time-domain surveys.
Sources
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- Neural Machine Translation by Jointly Learning to Align and Translate
- Making Better Mistakes: Leveraging Class Hierarchies with Deep Networks
- Astro-MoE: Mixture of Experts for Multiband Astronomical Time Series
- Astronomical Classification of Light Curves with an Ensemble of Gated Recurrent Units
- The Pan-STARRS1 Surveys
- On the Properties of Neural Machine Translation: Encoder-Decoder Approaches
- The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
- Minuet: A Diffusion Autoencoder for Compact Semantic Compression of Multi-Band Galaxy Images
- Gaussian Error Linear Units (GELUs)
- Distilling the Knowledge in a Neural Network
- BOOM and Babamul: a real-time, multi-survey, optical alert broker system operating at scale
- Applying multimodal learning to Classify transient Detections Early (AppleCiDEr) I: Data set, methods, and infrastructure
- Adam: A Method for Stochastic Optimization
- Towards An Integrated Optical Transient Utility
- StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars
- A ConvNet for the 2020s
- Opportunities in AI/ML for the Rubin LSST Dark Energy Science Collaboration
- UMAP: Uniform Manifold Approximation and Projection for Dimension Reduction
- AION-1: Omnimodal Foundation Model for Astronomical Sciences
Related papers
- A signal dedispersion algorithm for imaging-based transient searches
- AVICA: A fully automated CASA pipeline for large volume VLBI data calibration
- Spectral Map Making with SPHEREx
- Long-Integration Magnetar Burst Observatory (LIMBO): Instrument Summary and Early FRB Rate Constraints
- Towards independent event horizon imaging of the supermassive black holes in M87 and the Milky Way
- A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline