A method for finding anomalous astronomical light curves and their analogues

Author:

Martínez-Galarza J Rafael1ORCID,Bianco Federica B2345,Crake Dennis167,Tirumala Kushal8,Mahabal Ashish A8ORCID,Graham Matthew J8ORCID,Giles Daniel9ORCID

Affiliation:

1. Center for Astrophysics | Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138, USA

2. Department of Physics and Astronomy, University of Delaware, 217 Sharp Lab, Newark DE 19716 USA

3. Joseph R. Biden, Jr. School of Public Policy and Administration, University of Delaware, 184 Academy St, Newark DE 19716 USA

4. University of Delaware Data Science Institute, 100 Discovery Blvd, Newark, DE 19713, USA

5. Center for Urban Science and Progress, New York University, 370 Jay St, Brooklyn NY 11201, USA

6. School of Physics and Astronomy, University of Southampton, Hampshire SO17 1BJ, UK

7. Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK

8. Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena CA 91125, USA

9. The SETI Institute. 189 Bernardo Ave, Suite 200, Mountain View CA 94043, USA

Abstract

ABSTRACT Our understanding of the Universe has profited from deliberate targeted studies of known phenomena, as well as from serendipitous unexpected discoveries, such as the discovery of a complex variability pattern in the direction of KIC 8462852 (Boyajian’s star). Upcoming surveys such as the Vera C. Rubin Observatory Legacy Survey of Space and Time will explore the parameter space of astrophysical transients at all time-scales, and offer the opportunity to discover even more extreme examples of unexpected phenomena. We investigate strategies to identify novel objects and to contextualize them within large time-series data sets in order to facilitate the discovery of new classes of objects as well as the physical interpretation of their anomalous nature. We develop a method that combines tree-based and manifold-learning algorithms for anomaly detection in order to perform two tasks: 1) identify and rank anomalous objects in a time-domain data set; and 2) group those anomalies according to their similarity in order to identify analogues. We achieve the latter by combining an anomaly score from a tree-based method with a dimensionality manifold-learning reduction strategy. Clustering in the reduced space allows for the successful identification of anomalies and analogues. We also assess the impact of pre-processing and feature engineering schemes and investigate the astrophysical nature of the objects that our models identify as anomalous by augmenting the Kepler data with Gaia colour and luminosity information. We find that multiple models, used in combination, are a promising strategy to identify novel light curves and light curve families.

Funder

Space Telescope Science Institute

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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