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Machine-learning Approaches to Exoplanet Transit Detection and Candidate Validation in Wide-field Ground-based Surveys

Schanche, N; Collier Cameron, A; Hébrard, G; Nielsen, L; Triaud, A H M J; Almenara, J M; Alsubai, K A; Anderson, D R; Armstrong, D J; Barros, S C C; Bouchy, F; Boumis, P; Brown, D J A; Faedi, F; Hay, K; Hebb, L; Kiefer, F; Mancini, L; Maxted, P F L; Palle, E; Pollacco, D L; Queloz, D; Smalley, B; Udry, S; West, R; Wheatley, P J

Machine-learning Approaches to Exoplanet Transit Detection and Candidate Validation in Wide-field Ground-based Surveys Thumbnail


Authors

N Schanche

A Collier Cameron

G Hébrard

L Nielsen

A H M J Triaud

J M Almenara

K A Alsubai

D R Anderson

D J Armstrong

S C C Barros

F Bouchy

P Boumis

D J A Brown

F Faedi

K Hay

L Hebb

F Kiefer

L Mancini

E Palle

D L Pollacco

D Queloz

S Udry

R West

P J Wheatley



Abstract

Since the start of the Wide Angle Search for Planets (WASP) program, more than 160 transiting exoplanets have been discovered in the WASP data. In the past, possible transit-like events identified by the WASP pipeline have been vetted by human inspection to eliminate false alarms and obvious false positives. The goal of the present paper is to assess the effectiveness of machine learning as a fast, automated, and reliable means of performing the same functions on ground-based wide-field transit-survey data without human intervention. To this end, we have created training and test datasets made up of stellar light curves showing a variety of signal types including planetary transits, eclipsing binaries, variable stars, and non-periodic signals. We use a combination of machine learning methods including Random Forest Classifiers (RFCs) and Convolutional Neural Networks (CNNs) to distinguish between the different types of signals. The final algorithms correctly identify planets in the test data ~90% of the time, although each method on its own has a significant fraction of false positives. We find that in practice, a combination of different methods offers the best approach to identifying the most promising exoplanet transit candidates in data from WASP, and by extension similar transit surveys.

Citation

Schanche, N., Collier Cameron, A., Hébrard, G., Nielsen, L., Triaud, A. H. M. J., Almenara, J. M., Alsubai, K. A., Anderson, D. R., Armstrong, D. J., Barros, S. C. C., Bouchy, F., Boumis, P., Brown, D. J. A., Faedi, F., Hay, K., Hebb, L., Kiefer, F., Mancini, L., Maxted, P. F. L., Palle, E., …Wheatley, P. J. (2018). Machine-learning Approaches to Exoplanet Transit Detection and Candidate Validation in Wide-field Ground-based Surveys. Monthly Notices of the Royal Astronomical Society, 483(4), 5534-5547. https://doi.org/10.1093/mnras/sty3146

Journal Article Type Article
Acceptance Date Nov 13, 2018
Online Publication Date Nov 22, 2018
Publication Date Nov 22, 2018
Publicly Available Date May 26, 2023
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 483
Issue 4
Pages 5534-5547
DOI https://doi.org/10.1093/mnras/sty3146
Keywords Earth and Planetary Astrophysics; Instrumentation and Methods for Astrophysics
Public URL https://keele-repository.worktribe.com/output/412210
Publisher URL https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/sty3146/5199219

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