English

A Bayesian quantification of consistency in correlated datasets

Cosmology and Nongalactic Astrophysics 2019-01-24 v2

Abstract

We present three tiers of Bayesian consistency tests for the general case of correlatedcorrelated datasets. Building on duplicates of the model parameters assigned to each dataset, these tests range from Bayesian evidence ratios as a global summary statistic, to posterior distributions of model parameter differences, to consistency tests in the data domain derived from posterior predictive distributions. For each test we motivate meaningful threshold criteria for the internal consistency of datasets. Without loss of generality we focus on mutually exclusive, correlated subsets of the same dataset in this work. As an application, we revisit the consistency analysis of the two-point weak lensing shear correlation functions measured from KiDS-450 data. We split this dataset according to large vs. small angular scales, tomographic redshift bin combinations, and estimator type. We do not find any evidence for significant internal tension in the KiDS-450 data, with significances below 3σ3\, \sigma in all cases. Software and data used in this analysis can be found at http://kids.strw.leidenuniv.nl/sciencedata.php

Keywords

Cite

@article{arxiv.1809.01406,
  title  = {A Bayesian quantification of consistency in correlated datasets},
  author = {Fabian Köhlinger and Benjamin Joachimi and Marika Asgari and Massimo Viola and Shahab Joudaki and Tilman Tröster},
  journal= {arXiv preprint arXiv:1809.01406},
  year   = {2019}
}

Comments

Accepted by MNRAS. Conclusions unchanged with respect to v1, but now a more pedagogical introduction to all consistency tests is included in (new) Section 3. Software and data used in this analysis are available at http://kids.strw.leidenuniv.nl/sciencedata.php

R2 v1 2026-06-23T03:54:50.449Z