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Locating Hidden Exoplanets in ALMA Data Using Machine Learning

Abstract:
Abstract Exoplanets in protoplanetary disks cause localized deviations from Keplerian velocity in channel maps of molecular line emission. Current methods of characterizing these deviations are time consuming,and there is no unified standard approach. We demonstrate that machine learning can quickly and accurately detect the presence of planets. We train our model on synthetic images generated from simulations and apply it to real observations to identify forming planets in real systems. Machine-learning methods, based on computer vision, are not only capable of correctly identifying the presence of one or more planets, but they can also correctly constrain the location of those planets.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/aca477

Authors

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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-8590-7271
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Role:
Author
ORCID:
0000-0002-8138-0425
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Role:
Author
ORCID:
0000-0002-9426-3789
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Role:
Author
ORCID:
0000-0002-6222-8102


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
941
Issue:
2
Pages:
192-192
Publication date:
2022-12-01
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


Language:
English
Keywords:
Pubs id:
2374151
Local pid:
pubs:2374151
Source identifiers:
W4312170921
Deposit date:
2026-02-15
ARK identifier:
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