Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison

Fuente: arXiv
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Main Authors: Zhou, Lingyi, Radev, Stefan T., Oliver, William H., Obreja, Aura, Jin, Zehao, Buck, Tobias
Format: Preprint
Published: 2024
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author Zhou, Lingyi
Radev, Stefan T.
Oliver, William H.
Obreja, Aura
Jin, Zehao
Buck, Tobias
author_facet Zhou, Lingyi
Radev, Stefan T.
Oliver, William H.
Obreja, Aura
Jin, Zehao
Buck, Tobias
contents Cosmological simulations are a powerful tool to advance our understanding of galaxy formation and many simulations model key properties of real galaxies. A question that naturally arises for such simulations in light of high-quality observational data is: How close are the models to reality? Due to the high-dimensionality of the problem, many previous studies evaluate galaxy simulations using simplified summary statistics of physical properties. In this work, we combine simulation-based Bayesian model comparison with a novel misspecification detection technique to compare simulated galaxy images of 6 hydrodynamical models observations. Since cosmological simulations are computationally costly, we address the problem of low simulation budgets by first training a $k$-sparse variational autoencoder (VAE) on the abundant dataset of SDSS images. The VAE learns to extract informative latent embeddings and delineates the typical set of real images. To reveal simulation gaps, we then perform out-of-distribution detection (OOD) based on the logits of classifiers trained on the embeddings of simulated images. Finally, we perform amortized Bayesian model comparison using probabilistic classification, identifying the relatively best-performing model along with partial explanations through SHAP values.
format Preprint
id arxiv_https___arxiv_org_abs_2410_10606
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
Zhou, Lingyi
Radev, Stefan T.
Oliver, William H.
Obreja, Aura
Jin, Zehao
Buck, Tobias
Astrophysics of Galaxies
Computational Physics
Data Analysis, Statistics and Probability
Space Physics
Cosmological simulations are a powerful tool to advance our understanding of galaxy formation and many simulations model key properties of real galaxies. A question that naturally arises for such simulations in light of high-quality observational data is: How close are the models to reality? Due to the high-dimensionality of the problem, many previous studies evaluate galaxy simulations using simplified summary statistics of physical properties. In this work, we combine simulation-based Bayesian model comparison with a novel misspecification detection technique to compare simulated galaxy images of 6 hydrodynamical models observations. Since cosmological simulations are computationally costly, we address the problem of low simulation budgets by first training a $k$-sparse variational autoencoder (VAE) on the abundant dataset of SDSS images. The VAE learns to extract informative latent embeddings and delineates the typical set of real images. To reveal simulation gaps, we then perform out-of-distribution detection (OOD) based on the logits of classifiers trained on the embeddings of simulated images. Finally, we perform amortized Bayesian model comparison using probabilistic classification, identifying the relatively best-performing model along with partial explanations through SHAP values.
title Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
topic Astrophysics of Galaxies
Computational Physics
Data Analysis, Statistics and Probability
Space Physics
url https://arxiv.org/abs/2410.10606