TL;DR
This study compares correlation function methods and full-field inference in cosmology, showing that field-level analysis provides significantly higher accuracy and precision, especially in non-Gaussian scenarios, with simulation-based inference reducing biases.
Contribution
It demonstrates the advantages of field-level inference over correlation functions in cosmology, highlighting the importance of data assimilation techniques and simulation-based methods.
Findings
Field-level analysis outperforms correlation functions in accuracy and precision.
Likelihood assumptions can introduce biases in correlation function analysis.
Simulation-based inference reduces biases and improves results.
Abstract
We present a comparative study of the accuracy and precision of correlation function methods and full-field inference in cosmological data analysis. To do so, we examine a Bayesian hierarchical model that predicts log-normal fields and their two-point correlation function. Although a simplified analytic model, the log-normal model produces fields that share many of the essential characteristics of the present-day non-Gaussian cosmological density fields. We use three different statistical techniques: (i) a standard likelihood-based analysis of the two-point correlation function; (ii) a likelihood-free (simulation-based) analysis of the two-point correlation function; (iii) a field-level analysis, made possible by the more sophisticated data assimilation technique. We find that (a) standard assumptions made to write down a likelihood for correlation functions can cause significant…
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