Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
Natal\'i S. M. de Santi, Francisco Villaescusa-Navarro, L. Raul, Abramo, Helen Shao, Lucia A. Perez, Tiago Castro, Yueying Ni, Christopher C., Lovell, Elena Hernandez-Martinez, Federico Marinacci, David N. Spergel, Klaus, Dolag, Lars Hernquist, Mark Vogelsberger

TL;DR
This paper evaluates the robustness of graph neural network-based field-level inference models for cosmological parameters when applied to galaxy catalogs affected by realistic observational systematic effects.
Contribution
It extends previous models to include observational effects like masking and velocity uncertainties, demonstrating their resilience on simulated galaxy catalogs.
Findings
Models maintain over 90% accuracy despite observational effects.
Systematic effects degrade but do not eliminate model performance.
Models are promising for real data application in cosmology.
Abstract
It has been recently shown that a powerful way to constrain cosmological parameters from galaxy redshift surveys is to train graph neural networks to perform field-level likelihood-free inference without imposing cuts on scale. In particular, de Santi et al. (2023) developed models that could accurately infer the value of from catalogs that only contain the positions and radial velocities of galaxies that are robust to uncertainties in astrophysics and subgrid models. However, observations are affected by many effects, including 1) masking, 2) uncertainties in peculiar velocities and radial distances, and 3) different galaxy selections. Moreover, observations only allow us to measure redshift, intertwining galaxies' radial positions and velocities. In this paper we train and test our models on galaxy catalogs, created from thousands of state-of-the-art hydrodynamic…
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Taxonomy
Topicsdemographic modeling and climate adaptation · Galaxies: Formation, Evolution, Phenomena
