Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
ChangHoon Hahn, Mohammadjavad Vakili, Kilian Walsh, Andrew P. Hearin,, David W. Hogg, Duncan Campbell

TL;DR
This paper demonstrates that Approximate Bayesian Computation (ABC) can effectively infer galaxy-halo connection parameters in large scale structure, offering a likelihood-free alternative to traditional Gaussian-based methods.
Contribution
The study shows ABC's feasibility for LSS parameter inference using a forward model and compares its results with traditional MCMC, highlighting its reliability and potential advantages.
Findings
ABC constraints match true HOD parameters in mock data
ABC provides consistent results with Gaussian likelihood methods
ABC is a viable likelihood-free inference approach for LSS
Abstract
Standard approaches to Bayesian parameter inference in large scale structure assume a Gaussian functional form (chi-squared form) for the likelihood. This assumption, in detail, cannot be correct. Likelihood free inferences such as Approximate Bayesian Computation (ABC) relax these restrictions and make inference possible without making any assumptions on the likelihood. Instead ABC relies on a forward generative model of the data and a metric for measuring the distance between the model and data. In this work, we demonstrate that ABC is feasible for LSS parameter inference by using it to constrain parameters of the halo occupation distribution (HOD) model for populating dark matter halos with galaxies. Using specific implementation of ABC supplemented with Population Monte Carlo importance sampling, a generative forward model using HOD, and a distance metric based on galaxy number…
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