Clara M Pennock
The VMC Survey – LI. Classifying extragalactic sources using a probabilistic random forest supervised machine learning algorithm
Pennock, Clara M; van Loon, Jacco Th; Cioni, Maria-Rosa L; Maitra, Chandreyee; Oliveira, Joana M; Craig, Jessica E M; Ivanov, Valentin D; Aird, James; Anih, Joy O; Cross, Nicholas J G; Dresbach, Francesca; de Grijs, Richard; Groenewegen, Martin A T
Authors
Jacobus Van Loon j.t.van.loon@keele.ac.uk
Maria-Rosa L Cioni
Chandreyee Maitra
Joana Maria Oliveira j.oliveira@keele.ac.uk
Jessica E M Craig
Valentin D Ivanov
James Aird
Joy O Anih
Nicholas J G Cross
Francesca Dresbach
Richard de Grijs
Martin A T Groenewegen
Abstract
We used a supervised machine learning algorithm (probabilistic random forest) to classify ∼130 million sources in the VISTA Survey of the Magellanic Clouds (VMC). We used multi-wavelength photometry from optical to far-infrared as features to be trained on, and spectra of Active Galactic Nuclei (AGN), galaxies and a range of stellar classes including from new observations with the Southern African Large Telescope (SALT) and SAAO 1.9m telescope. We also retain a label for sources that remain unknown. This yielded average classifier accuracies of ∼79% (SMC) and ∼87% (LMC). Restricting to the 56,696,719 sources with class probabilities (Pclass) > 80% yields accuracies of ∼90% (SMC) and ∼98% (LMC). After removing sources classed as ‘Unknown’, we classify a total of 707,939 (SMC) and 397,899 (LMC) sources, including >77,600 extragalactic sources behind the Magellanic Clouds. The extragalactic sources are distributed evenly across the field, whereas the Magellanic sources concentrate at the centres of the Clouds, and both concentrate in optical/IR colour–colour/magnitude diagrams as expected. We also test these classifications using independent datasets, finding that, as expected, the majority of X-ray sources are classified as AGN (554/883) and the majority of radio sources are classed as AGN (1756/2694) or galaxies (659/2694), where the relative AGN–galaxy proportions vary substantially with radio flux density. We have found: >49,500 hitherto unknown AGN candidates, likely including more AGN dust dominated sources which are in a critical phase of their evolution; >26,500 new galaxy candidates and >2800 new Young Stellar Object (YSO) candidates.
Citation
Pennock, C. M., van Loon, J. T., Cioni, M.-R. L., Maitra, C., Oliveira, J. M., Craig, J. E. M., …Groenewegen, M. A. T. (2025). The VMC Survey – LI. Classifying extragalactic sources using a probabilistic random forest supervised machine learning algorithm. Monthly Notices of the Royal Astronomical Society, 537(2), 1028-1055. https://doi.org/10.1093/mnras/staf080
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 10, 2025 |
Online Publication Date | Jan 15, 2025 |
Publication Date | 2025-02 |
Deposit Date | Feb 3, 2025 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 537 |
Issue | 2 |
Pages | 1028-1055 |
DOI | https://doi.org/10.1093/mnras/staf080 |
Keywords | methods: data analysis, galaxies: active, Magellanic Clouds, galaxies: photometry |
Public URL | https://keele-repository.worktribe.com/output/1053698 |
Publisher URL | https://academic.oup.com/mnras/article/537/2/1028/7954762?login=true |
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