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20232026
most citedGalaxy Clustering Analysis with SimBIG and the Wavelet Scattering Transform

33 citations · 77 across the 16 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.IM2025

Semantic search for 100M+ galaxy images using AI-generated captions

Nolan Koblischke, Liam Parker, Francois Lanusse +3

Finding scientifically interesting phenomena through slow manual labeling campaigns severely limits our ability to explore the billions of galaxy images produced by telescopes. In…

cs.LG2025

Predicting partially observable dynamical systems via diffusion models with a multiscale inference scheme

Rudy Morel, Francesco Pio Ramunno, Jeff Shen +18

Conditional diffusion models provide a natural framework for probabilistic prediction of dynamical systems and have been successfully applied to fluid dynamics and weather predicti…

astro-ph.IM2025

Universal Spectral Tokenization via Self-Supervised Panchromatic Representation Learning

Jeff Shen, Francois Lanusse, Liam Holden Parker +24

Sequential scientific data span many resolutions and domains, and unifying them into a common representation is a key step toward developing foundation models for the sciences. Ast…

cs.LG2025

Walrus: A Cross-Domain Foundation Model for Continuum Dynamics

Michael McCabe, Payel Mukhopadhyay, Tanya Marwah +22

Foundation models have transformed machine learning for language and vision, but achieving comparable impact in physical simulation remains a challenge. Data heterogeneity and unst…

astro-ph.IM2025

AION-1: Omnimodal Foundation Model for Astronomical Sciences

Liam Parker, Francois Lanusse, Jeff Shen +24

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 th…

astro-ph.CO2025★ 1 cited

Initial Conditions from Galaxies: Machine-Learning Subgrid Correction to Standard Reconstruction

Liam Parker, Adrian E. Bayer, Uros Seljak

We present a hybrid method for reconstructing the primordial density from late-time halos and galaxies. Our approach involves two steps: (1) apply standard Baryon Acoustic Oscillat…