Published March 2026 | Version Published
Journal Article Open

Large Language Model–driven Analysis of General Coordinates Network (GCN) Circulars

  • 1. ROR icon Goddard Space Flight Center
  • 2. ROR icon University of Maryland, Baltimore County
  • 3. ROR icon University of California, San Diego
  • 4. ROR icon University of Maryland, College Park
  • 5. ROR icon University of Minnesota
  • 6. ROR icon Louisiana State University
  • 7. ROR icon Adnet Systems (United States)
  • 8. ROR icon California Institute of Technology
  • 9. ROR icon Massachusetts Institute of Technology
  • 10. ROR icon AI Institute for Artificial Intelligence and Fundamental Interactions

Abstract

The General Coordinates Network (GCN) is NASA's time-domain and multimessenger alert system. GCN distributes two data products: automated "Notices" and human-generated "Circulars" that report the observations of high-energy and multimessenger astronomical transients. The flexible and nonstructured format of GCN Circulars, comprising more than 40,500 Circulars accumulated over three decades, makes it challenging to manually extract observational information, such as redshift or observed wave bands. In this work, we employ large language models (LLMs) to facilitate the automated parsing of transient reports. We develop a neural topic modeling pipeline with open-source tools for the automatic clustering and summarization of astrophysical topics in the Circulars archive. Using neural topic modeling and contrastive fine-tuning, we classify Circulars based on their observation wave bands and messengers. Additionally, we separate gravitational-wave event clusters and their electromagnetic counterparts from the Circulars archive. Finally, using the open-source Mistral model, we implement a system to automatically extract gamma-ray burst (GRB) redshift information from the Circulars archive, without the need for any training. Evaluation against the manually curated Neil Gehrels Swift Observatory GRB table shows that our simple system, with the help of prompt-tuning, output parsing, and retrieval augmented generation (RAG), can achieve an accuracy of 97.2% for redshift-containing Circulars. Our neural search-enhanced RAG pipeline accurately retrieved 96.8% of redshift Circulars from the manually curated archive. Our study demonstrates the potential of LLMs to automate and enhance astronomical text mining and provides a foundational work for future advances in transient alert analysis.

Copyright and License

© 2026. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Acknowledgement

We thank the anonymous referee for useful comments and suggestions on the manuscript. V.S. was sponsored by support from NASA through a cooperative agreement with the Center for Research and Exploration in Space Science and Technology II (CRESST II). The views and conclusions contained in this document are those of the authors and should not be interpreted as representing the official policies, either expressed or implied, of NASA or the US Government. The US Government is authorized to reproduce and distribute reprints for Government purposes, notwithstanding any copyright notation herein. The GCN team acknowledges support from NASA’s Internal Scientist Funding Model (ISFM) program. This research has made use of data obtained through the GCN Service, provided by the NASA Goddard Space Flight Center (GSFC), in support of NASA’s High Energy Astrophysics Programs. The authors would also like to thank Daniela Huppenkothen for the insightful discussions. R.G. was sponsored by NASA through a contract with ORAU. M.W.C. acknowledges support from the National Science Foundation (NSF) under grant Nos. PHY-2409481, PHY-2308862, and PHY-2117997. N.M. acknowledges support from NSF under awards PHY-1764464 and PHY-2309200 to the LIGO Laboratory, under Cooperative Agreement PHY-2019786 (The NSF AI Institute for Artificial Intelligence and Fundamental Interactions, http://iaifi.org/), and from MathWorks, Inc.

Code Availability

All codes are available to the wider astrophysical community via Zenodo (doi:10.5281/zenodo.17538208) and the GitHub public repository19 at nasa-gcn. The repositories contain data, figures, and code in the Google Colab notebooks and extended tables.

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Additional details

Related works

Is new version of
Discussion Paper: arXiv:2511.14858 (arXiv)

Funding

National Aeronautics and Space Administration
Oak Ridge Associated Universities
National Science Foundation
PHY-2409481
National Science Foundation
PHY-2308862
National Science Foundation
PHY-2117997
National Science Foundation
PHY-1764464
National Science Foundation
PHY-2309200
National Science Foundation
PHY-2019786

Dates

Submitted
2025-10-20
Accepted
2025-11-18
Available
2026-02-27
Published