An approach to robust Bayesian regression in astronomy
William Martin, Daniel J. Mortlock

TL;DR
This paper introduces a robust Bayesian linear regression method using Student's t-distributions, effectively handling outliers and model mis-specification in astronomical data analysis, with validated performance on simulated and real datasets.
Contribution
Develops a generic Bayesian regression approach based on Student's t-distributions that is robust to outliers and noise model mis-specification, and provides a Python implementation.
Findings
Less biased parameter constraints compared to normal distribution models.
Unbiased results with minimal uncertainty increase for outlier-free data.
Qualitative differences in results when compared to traditional methods.
Abstract
Model mis-specification (e.g. the presence of outliers) is commonly encountered in astronomical analyses, often requiring the use of ad hoc algorithms which are sensitive to arbitrary thresholds (e.g. sigma-clipping). For any given dataset, the optimal approach will be to develop a bespoke statistical model of the data generation and measurement processes, but these come with a development cost; there is hence utility in having generic modelling approaches that are both principled and robust to model mis-specification. Here we develop and implement a generic Bayesian approach to linear regression, based on Student's t-distributions, that is robust to outliers and mis-specification of the noise model. Our method is validated using simulated datasets with various degrees of model mis-specification; the derived constraints are shown to be systematically less biased than those from a…
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Taxonomy
TopicsSpectroscopy and Chemometric Analyses · Fault Detection and Control Systems · Gaussian Processes and Bayesian Inference
