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This research advances the computational efficiency of scan statistics by reducing complexity from $O(n^4)$ to linear time using kernel regression techniques. The approach offers significant practical value for detecting anomalies in non-stationary real-valued signals, with demonstrated applications ranging from synthetic data to interferometric astronomy. By enabling faster processing of large datasets, these models facilitate more scalable statistical monitoring and outlier detection in complex scientific domains.
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Efficient Regression Models for Scan Statistics

arXiv1 min read

arXiv:2608.22201v1 Announce Type: cross Abstract: We introduce a new class of regression models for scan statistics on real-valued signals. These allow for improved fitting of non-stationary signals to contrast with the interval anomalies identified by the scan statistics. Our models can represent generalized likelihood ratio statistics. While these methods naively require $O(n^4)$ for a length $n$ signal, we provide algorithmic improvements which lead to linear time algorithms (with assumptions on max interval width). Our methods, especially ones based on Nadaraya-Watson kernel regression, are demonstrated as especially effective in detecting both synthetically planted anomalies, and for identifying a real ``platforming'' issue in interferometric astronomy.

Abstract:We introduce a new class of regression models for scan statistics on real-valued signals. These allow for improved fitting of non-stationary signals to contrast with the interval anomalies identified by the scan statistics. Our models can represent generalized likelihood ratio statistics. While these methods naively require $O(n^4)$ for a length $n$ signal, we provide algorithmic improvements which lead to linear time algorithms (with assumptions on max interval width). Our methods, especially ones based on Nadaraya-Watson kernel regression, are demonstrated as especially effective in detecting both synthetically planted anomalies, and for identifying a real ``platforming'' issue in interferometric astronomy.

Methodology (stat.ME); Machine Learning (cs.LG)

arXiv:2608.22201 [stat.ME]

(or arXiv:2608.22201v1 [stat.ME] for this version)

https://doi.org/10.48550/arXiv.2608.22201 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 194 words

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