Multiscale Flow for Robust and Optimal Cosmological Analysis
Biwei Dai, Uros Seljak

TL;DR
Multiscale Flow is a hierarchical generative model for cosmological data that improves likelihood estimation, detects distribution shifts, and generates realistic weak lensing samples, outperforming traditional methods.
Contribution
It introduces a wavelet-based hierarchical Normalizing Flow that models field-level likelihoods in cosmology, enabling optimal analysis and shift detection without dimensionality reduction.
Findings
Outperforms traditional summary statistics in cosmological inference
Identifies distribution shifts like baryonic effects in data
Generates realistic weak lensing data samples
Abstract
We propose Multiscale Flow, a generative Normalizing Flow that creates samples and models the field-level likelihood of two-dimensional cosmological data such as weak lensing. Multiscale Flow uses hierarchical decomposition of cosmological fields via a wavelet basis, and then models different wavelet components separately as Normalizing Flows. The log-likelihood of the original cosmological field can be recovered by summing over the log-likelihood of each wavelet term. This decomposition allows us to separate the information from different scales and identify distribution shifts in the data such as unknown scale-dependent systematics. The resulting likelihood analysis can not only identify these types of systematics, but can also be made optimal, in the sense that the Multiscale Flow can learn the full likelihood at the field without any dimensionality reduction. We apply Multiscale…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories
MethodsNormalizing Flows
