Measurement errors and scaling relations in astrophysics: a review

Abstract

This review article considers some of the most common methods used in astronomy for regressing one quantity against another in order to estimate the model parameters or to predict an observationally expensive quantity using trends between object values. These methods have to tackle some of the awkward features prevalent in astronomical data, namely heteroscedastic (point-dependent) errors, intrinsic scatter, non-ignorable data collection and selection effects, data structure and non-uniform population (often called Malmquist bias), non-Gaussian data, outliers and mixtures of regressions. We outline how least square fits, weighted least squares methods, Maximum Likelihood, survival analysis, and Bayesian methods have been applied in the astrophysics literature when one or more of these features is present. In particular we concentrate on errors-in-variables regression and we advocate Bayesian techniques.

Invited review on "Statistical Analysis and Data Mining", a referred journal of the American Statistical Association. In press

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Cited by in corpus (6)

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• Comparing Masses in Literature (CoMaLit)-I. Bias and scatter in weak lensing and X-ray mass estimates of clusters
• A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars
• The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects
• CoMaLit - II. The scaling relation between mass and Sunyaev-Zel'dovich signal for Planck selected galaxy clusters
• Non-Gaussian Error Distributions of LMC Distance Moduli Measurements