Influence function Created 2026-09-24 Updated 2026-10-14
An influence function asks how much a population answer moves when an infinitesimal fraction of its probability distribution is relocated to a specified point. It distinguishes the unbounded response of the mean from the bounded response of the median and the Huber location estimator. The normal-location influence curves and finite contamination bias of normal location below make that difference quantitative.
Let be a real-valued statistical functional, a reference probability measure, and the Dirac measure concentrated at . Along the epsilon-contamination neighborhood path , define the right derivativeThe name influence curve refers to the same object. The derivative is in the signed direction , so the calculation removes baseline mass as well as adding a Dirac measure. The definition is a limit for each fixed ; it does not automatically give a remainder uniform over arbitrarily distant .[ref]
The Influence Curve and Its Role in Robust Estimation by Frank R. Hampel. Frank R. Hampel, The Influence Curve and Its Role in Robust Estimation, p. 383, §2: pointwise right-limit definition along mixtures with a point mass
The statistical functional must be defined on these contaminated probability measures, and the right derivative must exist and be finite. For a mean, a finite first absolute moment suffices. For a median, require a unique baseline median and a probability density function continuous and strictly positive there. For a smooth M-estimator, require an isolated population root, justified differentiation of its expected value, and a nonzero derivative with respect to the fitted parameter. These are specific conditions for the formulas below. Existence of the pointwise influence function alone proves neither an asymptotic linear representation nor pathwise differentiability of a statistical functional; each needs control of its own remainder and admissible statistical paths.
Local influence versus replacement breakdown 2026-10-14
The influence function describes an infinitesimal change at a specified reference probability distribution. The replacement breakdown point asks how many observations in a particular finite sample can be replaced before an estimator becomes unbounded. The finite-sample maximum bias records the intervening changes. These are different questions: a bounded influence function at one baseline is not a general bound over all epsilon-contamination neighborhoods, nor a proof of a positive replacement breakdown point.[ref]
The Influence Curve and Its Role in Robust Estimation by Frank R. Hampel. Frank R. Hampel, The Influence Curve and Its Role in Robust Estimation, §4, p. 386: exact asymptotic curve supplemented by behavior at other distributions, especially empirical ones
The mean illustrates agreement between local and global fragility: its gross-error sensitivity is infinite and one replacement can send the sample mean arbitrarily far. The median has finite gross-error sensitivity under the stated positive-density assumptions, while its sample median withstands fewer than about half the observations being replaced under ordinary tie conventions. Its population contamination bias above still diverges as when the atom remains beyond the shifted median. Here must also move outward; taking that limit with a fixed finite atom would invalidate the displayed quantile formula.
For scalar location with a fixed positive scale, the Huber score has a direct global argument: if strictly more than half of the sample stays fixed, then beyond every retained observation by more than , their saturated scores outweigh all possible replaced scores. Every root therefore stays in a bounded interval. This is a separate finite-replacement argument; estimating scale changes its premises. A smooth bounded influence function is valuable local protection, but global robustness also depends on the full estimating rule, scale choice, and root selection.
Past exam of the mathematics course of the University of Cambridge 2024 iii Paper 223 3 d Solution Created 2026-09-24 Updated 2026-09-25
For and , the nominal log-likelihood ratio for one observation is . Under sufficiently small epsilon-contamination neighborhoods, the least-favourable pair clips this likelihood ratio between two constants. Symmetry turns its log into a positive multiple of the winsorized scoreThe robust form of the Neyman-Pearson lemma therefore rejects for large values ofwith boundary randomization and threshold chosen so that the worst-case null rejection probability is . Extreme observations contribute only , preventing a few contaminants from dominating the test.