# Sparse Bayesian mass-mapping with uncertainties: hypothesis testing of   structure

**Authors:** Matthew A. Price, Jason D. McEwen, Xiaohao Cai, Thomas D. Kitching,, Christopher G. R. Wallis (for the LSST Dark Energy Science Collaboration)

arXiv: 1812.04014 · 2021-12-16

## TL;DR

This paper introduces a Bayesian mass-mapping method that quantifies uncertainties and enables hypothesis testing of structures, improving the reliability of weak lensing reconstructions without assuming Gaussianity.

## Contribution

The authors develop a convex optimization-based Bayesian framework for mass-mapping that provides conservative uncertainty estimates and hypothesis testing capabilities for structures.

## Key findings

- Method successfully applied to simulations and observational data.
- Neither dataset conclusively confirms the dark core hypothesis at 99% confidence.
- Reconstructed maps are consistent with observational data.

## Abstract

A crucial aspect of mass-mapping, via weak lensing, is quantification of the uncertainty introduced during the reconstruction process. Properly accounting for these errors has been largely ignored to date. We present a new method to reconstruct maximum a posteriori (MAP) convergence maps by formulating an unconstrained Bayesian inference problem with Laplace-type l1-norm sparsity-promoting priors, which we solve via convex optimization. Approaching mass-mapping in this manner allows us to exploit recent developments in probability concentration theory to infer theoretically conservative uncertainties for our MAP reconstructions, without relying on assumptions of Gaussianity. For the first time these methods allow us to perform hypothesis testing of structure, from which it is possible to distinguish between physical objects and artifacts of the reconstruction. Here we present this new formalism, demonstrate the method on simulations, before applying the developed formalism to two observational datasets of the Abel-520 cluster. Initial reconstructions of the Abel-520 catalogs reported the detection of an anomalous 'dark core' -- an over dense region with no optical counterpart -- which was taken to be evidence for self-interacting dark-matter. In our Bayesian framework it is found that neither Abel-520 dataset can conclusively determine the physicality of such dark cores at 99% confidence. However, in both cases the recovered MAP estimators are consistent with both sets of data.

## Full text

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## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/1812.04014/full.md

## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1812.04014/full.md

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Source: https://tomesphere.com/paper/1812.04014