Jiani Chu
Galaxy stellar and total mass estimation using machine learning
Chu, Jiani; Tang, Hongming; Xu, Dandan; Lu, Shengdong; Long, Richard
Authors
Hongming Tang
Dandan Xu
Dr Shengdong Lu shengdong.lu@durham.ac.uk
Postdoctoral Research Associate
Richard Long
Abstract
Conventional galaxy mass estimation methods suffer from model assumptions and degeneracies. Machine learning (ML), which reduces the reliance on such assumptions, can be used to determine how well present-day observations can yield predictions for the distributions of stellar and dark matter. In this work, we use a general sample of galaxies from the TNG100 simulation to investigate the ability of multibranch convolutional neural network (CNN) based ML methods to predict the central (i.e. within 1−2 effective radii) stellar and total masses, and the stellar mass-to-light ratio (M*/L). These models take galaxy images and spatially resolved mean velocity and velocity dispersion maps as inputs. Such CNN-based models can, in general, break the degeneracy between baryonic and dark matter in the sense that the model can make reliable predictions on the individual contributions of each component. For example, with r-band images and two galaxy kinematic maps as inputs, our model predicting M*/L has a prediction uncertainty of 0.04 dex. Moreover, to investigate which (global) features significantly contribute to the correct predictions of the properties above, we utilize a gradient-boosting machine. We find that galaxy luminosity dominates the prediction of all masses in the central regions, with stellar velocity dispersion coming next. We also investigate the main contributing features when predicting stellar and dark matter mass fractions (f*, fDM) and the dark matter mass MDM, and discuss the underlying astrophysics.
Citation
Chu, J., Tang, H., Xu, D., Lu, S., & Long, R. (2024). Galaxy stellar and total mass estimation using machine learning. Monthly Notices of the Royal Astronomical Society, 528(4), 6354-6369. https://doi.org/10.1093/mnras/stae406
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 30, 2024 |
Online Publication Date | Feb 7, 2024 |
Publication Date | 2024-03 |
Deposit Date | Mar 12, 2024 |
Publicly Available Date | Mar 12, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 528 |
Issue | 4 |
Pages | 6354-6369 |
DOI | https://doi.org/10.1093/mnras/stae406 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://durham-repository.worktribe.com/output/2326259 |
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Copyright Statement
© 2024 The Author(s).
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,
provided the original work is properly cited.
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