Finding Anomalous Periodic Time Series: An Application to Catalogs of Periodic Variable Stars

TL;DR

This paper introduces PCAD, an unsupervised anomaly detection method tailored for large, unsynchronized periodic time series data, such as light-curves of variable stars, effectively identifying both global and local anomalies without requiring costly alignment.

Contribution

The paper presents PCAD, a scalable anomaly detection approach that handles unsynchronized periodic time series using a modified k-means clustering and sampling, outperforming existing methods.

Findings

PCAD effectively detects known and novel anomalies in astrophysical data.

Sampling and number of centroids influence detection accuracy.

PCAD's anomalies are validated by astrophysicists as potentially new phenomena.

Abstract

Catalogs of periodic variable stars contain large numbers of periodic light-curves (photometric time series data from the astrophysics domain). Separating anomalous objects from well-known classes is an important step towards the discovery of new classes of astronomical objects. Most anomaly detection methods for time series data assume either a single continuous time series or a set of time series whose periods are aligned. Light-curve data precludes the use of these methods as the periods of any given pair of light-curves may be out of sync. One may use an existing anomaly detection method if, prior to similarity calculation, one performs the costly act of aligning two light-curves, an operation that scales poorly to massive data sets. This paper presents PCAD, an unsupervised anomaly detection method for large sets of unsynchronized periodic time-series data, that outputs a ranked list of both global and local anomalies. It calculates its anomaly score for each light-curve in relation to a set of centroids produced by a modified k-means clustering algorithm. Our method is able to scale to large data sets through the use of sampling. We validate our method on both light-curve data and other time series data sets. We demonstrate its effectiveness at finding known anomalies, and discuss the effect of sample size and number of centroids on our results. We compare our method to naive solutions and existing time series anomaly detection methods for unphased data, and show that PCAD's reported anomalies are comparable to or better than all other methods. Finally, astrophysicists on our team have verified that PCAD finds true anomalies that might be indicative of novel astrophysical phenomena.