Searching for bias and correlations in a Bayesian way
Caroline Heneka (Dark Cosmology Ctr.), Alexandre Posada (U., Aix-Marseille, CPT), Valerio Marra (U. Fed. Rio de Janeiro, Inst. Phys.),, Luca Amendola (U. Heidelberg, ITP)

TL;DR
This paper introduces a Bayesian approach using internal robustness to detect biases and hidden correlations in large cosmological datasets, enhancing measurement accuracy in a model-independent manner.
Contribution
It extends previous methods by applying internal robustness to identify biased data subsets and correlations without relying on specific models.
Findings
Effective detection of biased data subsets
Identification of hidden correlations in datasets
Improved accuracy in cosmological parameter inference
Abstract
A range of Bayesian tools has become widely used in cosmological data treatment and parameter inference (see Kunz, Bassett & Hlozek (2007), Trotta (2008), Amendola, Marra & Quartin (2013)). With increasingly big datasets and higher precision, tools that enable us to further enhance the accuracy of our measurements gain importance. Here we present an approach based on internal robustness, introduced in Amendola, Marra & Quartin (2013) and adopted in Heneka, Marra & Amendola (2014), to identify biased subsets of data and hidden correlation in a model independent way.
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