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AION-1: Omnimodal Foundation Model for Astronomical Sciences

Authors

  • Liam Parker
  • Francois Lanusse
  • Jeff Shen
  • Ollie Liu
  • Tom Hehir
  • Leopoldo Sarra
  • Lucas Meyer
  • Micah Bowles
  • Sebastian Wagner-Carena
  • Helen Qu
  • Siavash Golkar
  • Alberto Bietti
  • Hatim Bourfoune
  • Nathan Casserau
  • Pierre Cornette
  • Keiya Hirashima
  • Geraud Krawezik
  • Ruben Ohana
  • Nicholas Lourie
  • Michael McCabe
  • Rudy Morel
  • Payel Mukhopadhyay
  • Mariel Pettee
  • Bruno Regaldo-Saint Blancard
  • Kyunghyun Cho
  • Miles Cranmer
  • Shirley Ho

Abstract

While foundation models have shown promise across a variety of fields, astronomy still lacks a unified framework for joint modeling across its highly diverse data modalities. In this paper, we present AION-1, a family of large-scale multimodal foundation models for astronomy. AION-1 integrates heterogeneous imaging, spectroscopic, and scalar data using a two-stage architecture: modality-specific tokenization followed by transformer-based masked modeling of cross-modal token sequences. The model is pretrained on five large-scale surveys: Legacy Survey, Hyper Suprime-Cam (HSC), Sloan Digital Sky Survey (SDSS), Dark Energy Spectroscopic Instrument (DESI), and Gaia. These span more than 200 million observations of stars, galaxies, and quasars. With a single frozen encoder, AION-1 achieves strong results on a broad suite of downstream tasks, including galaxy and stellar property estimation, galaxy morphology classification, similarity-based retrieval, galaxy image segmentation, and spectral super-resolution. We release AION-1 model variants ranging from 300 M to 3.1 B parameters. Beyond astronomy, AION-1 provides a scalable blueprint for multimodal scientific foundation models that can seamlessly integrate noisy, instrument-specific observations. All code, tokenizers, pretrained weights, and a lightweight evaluation suite are released under an open-source license.

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Posted

2025-10-20