Benne W. Holwerda
Galaxy and mass assembly (GAMA): Self-Organizing Map application on nearby galaxies
Holwerda, Benne W.; Smith, Dominic; Porter, Lori; Henry, Chris; Porter-Temple, Ren; Cook, Kyle; Pimbblet, Kevin A.; Hopkins, Andrew M; Bilicki, Maciej; Turner, Sebastian; Acquaviva, Viviana; Wang, Lingyu; Wright, Angus H.; Kelvin, Lee S.; Grootes, Meiert W
Authors
Dominic Smith
Lori Porter
Chris Henry
Ren Porter-Temple
Kyle Cook
Professor Kevin Pimbblet K.Pimbblet@hull.ac.uk
Director of DAIM
Andrew M Hopkins
Maciej Bilicki
Sebastian Turner
Viviana Acquaviva
Lingyu Wang
Angus H. Wright
Lee S. Kelvin
Meiert W Grootes
Abstract
Galaxy populations show bimodality in a variety of properties: stellar mass, colour, specific star-formation rate, size, and Sérsic index. These parameters are our feature space. We use an existing sample of 7556 galaxies from the Galaxy and Mass Assembly (GAMA) survey, represented using five features and the K-means clustering technique, showed that the bimodalities are the manifestation of a more complex population structure, represented by between two and six clusters. Here we use Self-Organizing Maps (SOM), an unsupervised learning technique that can be used to visualize similarity in a higher dimensional space using a 2D representation, to map these 5D clusters in the feature space on to 2D projections. To further analyse these clusters, using the SOM information, we agree with previous results that the sub-populations found in the feature space can be reasonably mapped on to three or five clusters. We explore where the 'green valley' galaxies are mapped on to the SOM, indicating multiple interstitial populations within the green valley population. Finally, we use the projection of the SOM to verify whether morphological information provided by GalaxyZoo users, for example, if features are visible, can be mapped on to the SOM-generated map. Voting on whether galaxies are smooth, likely ellipticals, or 'featured' can reasonably be separated but smaller morphological features (bar, spiral arms) can not. SOMs promise to be a useful tool to map and identify instructive sub-populations in multidimensional galaxy survey feature space, provided they are large enough.
Citation
Holwerda, B. W., Smith, D., Porter, L., Henry, C., Porter-Temple, R., Cook, K., …Grootes, M. W. (2022). Galaxy and mass assembly (GAMA): Self-Organizing Map application on nearby galaxies. Monthly notices of the Royal Astronomical Society, 513(2), 1972-1984. https://doi.org/10.1093/mnras/stac889
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 29, 2022 |
Online Publication Date | Apr 14, 2022 |
Publication Date | Jun 1, 2022 |
Deposit Date | Jun 16, 2022 |
Publicly Available Date | Jun 28, 2022 |
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 | 513 |
Issue | 2 |
Pages | 1972-1984 |
DOI | https://doi.org/10.1093/mnras/stac889 |
Keywords | Catalogues; Surveys; Galaxies: evolution; Galaxies: fundamental parameters; Galaxies: star formation; Galaxies: statistics |
Public URL | https://hull-repository.worktribe.com/output/3970443 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2022 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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