On the Significance of Covariance for Constraining Theoretical Models From Galaxy Observables
Yongseok Jo, Shy Genel, Joel Leja, Benjamin Wandelt

TL;DR
This paper examines how different covariance structures in uncertainties influence the inference of cosmological parameters from galaxy data, highlighting the importance of covariance modeling for accurate astrophysical analysis.
Contribution
It introduces a comprehensive analysis of covariance effects on parameter inference using forward modeling and emulators with CAMELS simulations, emphasizing the significance of covariance in astrophysical data interpretation.
Findings
Covariance significantly affects parameter constraints.
Different covariance models can lead to tighter or multimodal posteriors.
Physically motivated covariances alter inference outcomes.
Abstract
In this study, we investigate the impact of covariance within uncertainties on the inference of cosmological and astrophysical parameters, specifically focusing on galaxy stellar mass functions derived from the CAMELS simulation suite. Utilizing both Fisher analysis and Implicit Likelihood Inference (ILI), we explore how different covariance structures, including simple toy models and physics-motivated uncertainties, affect posterior distributions and parameter variances. Our methodology utilizes forward modeling via emulators that are trained on CAMELS simulations to produce stellar mass functions based on input parameters, subsequently incorporating Gaussian noise as defined by covariance matrices. We examine both toy model covariance matrices and physically motivated covariance matrices derived from observational factors like the stellar Initial Mass Function (IMF) and photometric…
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