Halo detection via large-scale Bayesian inference

TL;DR

This paper introduces a Bayesian method combining large-scale structure inference and a chain rule to detect dark matter halos in noisy cosmological data, validated with mock galaxy catalogues.

Contribution

It presents a novel Bayesian framework that links density inference to halo detection, enabling probabilistic maps of halo presence in cosmological observations.

Findings

Detection probability increases with signal-to-noise ratio.

Method accurately infers 3D density fields and uncertainties.

Validates approach with realistic mock galaxy data.

Abstract

We present a proof-of-concept of a novel and fully Bayesian methodology designed to detect halos of different masses in cosmological observations subject to noise and systematic uncertainties. Our methodology combines the previously published Bayesian large-scale structure inference algorithm, HADES, and a Bayesian chain rule (the Blackwell-Rao Estimator), which we use to connect the inferred density field to the properties of dark matter halos. To demonstrate the capability of our approach we construct a realistic galaxy mock catalogue emulating the wide-area 6-degree Field Galaxy Survey, which has a median redshift of approximately 0.05. Application of HADES to the catalogue provides us with accurately inferred three-dimensional density fields and corresponding quantification of uncertainties inherent to any cosmological observation. We then use a cosmological simulation to relate the amplitude of the density field to the probability of detecting a halo with mass above a specified threshold. With this information we can sum over the HADES density field realisations to construct maps of detection probabilities and demonstrate the validity of this approach within our mock scenario. We find that the probability of successful of detection of halos in the mock catalogue increases as a function of the signal-to-noise of the local galaxy observations. Our proposed methodology can easily be extended to account for more complex scientific questions and is a promising novel tool to analyse the cosmic large-scale structure in observations.