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Artificial Intelligence and Machine Learning Science and Technology Interest Group

The NASA Cosmic Origins Program AI/ML Science and Technology Interest Group (AI/ML STIG) addresses the critical need to upskill the astronomy community with AI literacy. We provide structured, domain-specific AI education through stackable, bite-sized modular training designed for astronomical research contexts.

About AI/ML STIG

Building AI Literacy for Astronomical Research

Astrophysics is an emerging technology for big-data science, and the use of Artificial Intelligence (AI) and Machine Learning (ML) technology will be inevitable in the coming decades.

The AI and ML Science and Technology Interest Group (AI/ML STIG) is motivated by the awareness that upskilling the scientific community could have a transformative impact to counter critical challenges facing astronomical research today.

Asteroid streaks found by AI in Hubble image
Astronomers have used AI and Hubble data to hunt asteroids in between the orbits of Mars and Jupiter. These small asteroids are faint and difficult to detect, but leave distinctive curved, streak-like trails on Hubble’s observations. These streaks left by asteroids on Hubble images are one of the items that artificial intelligence programs can sort through vast amounts of data to help identify.
NASA, ESA, and B. Sunnquist and J. Mack (STScI) Acknowledgment: NASA, ESA, and J. Lotz (STScI) and the HFF Team

By providing structured, domain-specific AI education, the AI/ML STIG aims to accelerate NASA's competitive advantage in AI-enabled space science, build the interdisciplinary workforce essential for next-generation astronomical discoveries, create a model for other NASA programs facing similar upskilling challenges, and establish NASA’s leadership in responsible AI adoption to maximize the science return from its missions by the community. The modular, community-driven approach ensures scalability while maintaining the rigor and domain relevance essential for meaningful scientific advancement. This STIG serves as a focal point for addressing these challenges through community townhalls for discussions and organizing short tutorials to address specific astronomical AI applications, modules, and foundational concepts.

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STIG Leadership

Yuan-Sen TingOSU
Alex GaglianoMIT
Siddharth Mishra-SharmaBoston University
Digvijay WadekarJohns Hopkins
Andrew SaydjariPrinceton
Carol Cuesta-LazaroMIT
Georgios ValogiannisUChicago

News & Events

Meetings, conferences, seminars, workshops, and other news and events for the STIG

AI/ML STIG Lecture Series, 13 April 2026

AI and Scientific Publishing. Speaker: Licia Verde, U. of Barcelona/JCAP

Apr 10, 2026
Topic
AI/ML STIG Lecture Series, 6 April 2026

Simulation-Based Inference Speaker Tomasz Rozanski, ANU An introduction to simulation-based inference (SBI) for astronomy, using normalizing flows to perform posterior estimation in settings where the likelihood is intractable. Hands-on tutorials cover a toy physics problem and a stellar population application.…

Apr 6, 2026
Topic
AI/ML STIG Lecture Series, 30 March 2026

Flow Matching Speaker Tomasz Rozanski, ANU A hands-on tutorial on flow matching for generative modeling in astronomy, covering continuous normalizing flows applied to stellar population modeling with both single and conditional population examples. Topics Covered Meeting Connection Join the Meeting

Mar 30, 2026
Topic
AI/ML STIG Lecture Series, 23 March 2026

Diffusion Models. Speaker Duo Xu, U. of Toronto

Mar 23, 2026
Topic
AI/ML STIG Lecture Series, 16 March 2026

Normalizing Flows Speaker Gregory Green, Westlake An introduction to normalizing flows for generative modeling, covering the mathematical foundations of invertible transformations and density estimation, with hands-on tutorials implementing RealNVP and flow matching techniques. Topics Covered Meeting Connection Join the Meeting

Mar 16, 2026
Topic
AI/ML STIG Lecture Series, 9 March 2026

Equivariant Neural Networks (Application) Speaker: Anna Scaife, U. of Manchester

Mar 9, 2026
Topic

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.