Unsupervised machine learning to detect anomalies

As survey astronomy continues to grow, the size and complexity of astronomical data bases will increase, and the ability of astronomers to manually scour data and make such discoveries decreases. In this work, we introduce a machine learning-based method to identify anomalies in large data sets to facilitate such discoveries, and apply this method to long cadence light curves from NASA's Kepler Mission.

Our method clusters data based on density, identifying anomalies as data that lie outside of dense regions. This work serves as a proof-of-concept case study and we test our method on four quarters of the Kepler long cadence light curves. We use Kepler's most notorious anomaly, Boyajian's star (KIC 8462852), as a rare 'ground truth' for testing outlier identification to verify that objects of genuine scientific interest are included among the identified anomalies.