Concentration bounds for the empirical angular measure with statistical learning applications

TL;DR

This paper establishes finite-sample concentration bounds for the empirical angular measure on the sphere, enabling reliable statistical learning in extreme regions with applications to classification and anomaly detection.

Contribution

It provides the first finite-sample bounds for the empirical angular measure, facilitating its use in statistical learning tasks involving extremes.

Findings

Bounds scale as the square root of effective sample size

High-probability uniform deviation bounds are derived

Applications include classification and anomaly detection

Abstract

The angular measure on the unit sphere characterizes the first-order dependence structure of the components of a random vector in extreme regions and is defined in terms of standardized margins. Its statistical recovery is an important step in learning problems involving observations far away from the center. In the common situation that the components of the vector have different distributions, the rank transformation offers a convenient and robust way of standardizing data in order to build an empirical version of the angular measure based on the most extreme observations. However, the study of the sampling distribution of the resulting empirical angular measure is challenging. It is the purpose of the paper to establish finite-sample bounds for the maximal deviations between the empirical and true angular measures, uniformly over classes of Borel sets of controlled combinatorial complexity. The bounds are valid with high probability and, up to logarithmic factors, scale as the square root of the effective sample size. The bounds are applied to provide performance guarantees for two statistical learning procedures tailored to extreme regions of the input space and built upon the empirical angular measure: binary classification in extreme regions through empirical risk minimization and unsupervised anomaly detection through minimum-volume sets of the sphere.