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Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies

Walmsley, Mike; Lintott, Chris; Géron, Tobias; Kruk, Sandor; Krawczyk, Coleman; Willett, Kyle W; Bamford, Steven; Kelvin, Lee S; Fortson, Lucy; Gal, Yarin; Keel, William; Masters, Karen L; Mehta, Vihang; Simmons, Brooke D; Smethurst, Rebecca; Smith, Lewis; Baeten, Elisabeth M; MacMillan, Christine

Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies Thumbnail


Authors

Mike Walmsley

Chris Lintott

Tobias Géron

Sandor Kruk

Coleman Krawczyk

Kyle W Willett

Lee S Kelvin

Lucy Fortson

Yarin Gal

William Keel

Karen L Masters

Vihang Mehta

Brooke D Simmons

Rebecca Smethurst

Lewis Smith

Elisabeth M Baeten

Christine MacMillan



Abstract

We present Galaxy Zoo DECaLS: detailed visual morphological classifications for Dark Energy Camera Legacy Survey images of galaxies within the SDSS DR8 footprint. Deeper DECaLS images (r = 23.6 versus r = 22.2 from SDSS) reveal spiral arms, weak bars, and tidal features not previously visible in SDSS imaging. To best exploit the greater depth of DECaLS images, volunteers select from a new set of answers designed to improve our sensitivity to mergers and bars. Galaxy Zoo volunteers provide 7.5 million individual classifications over 314 000 galaxies. 140 000 galaxies receive at least 30 classifications, sufficient to accurately measure detailed morphology like bars, and the remainder receive approximately 5. All classifications are used to train an ensemble of Bayesian convolutional neural networks (a state-of-the-art deep learning method) to predict posteriors for the detailed morphology of all 314 000 galaxies. We use active learning to focus our volunteer effort on the galaxies which, if labelled, would be most informative for training our ensemble. When measured against confident volunteer classifications, the trained networks are approximately 99 per cent accurate on every question. Morphology is a fundamental feature of every galaxy; our human and machine classifications are an accurate and detailed resource for understanding how galaxies evolve.

Citation

Walmsley, M., Lintott, C., Géron, T., Kruk, S., Krawczyk, C., Willett, K. W., Bamford, S., Kelvin, L. S., Fortson, L., Gal, Y., Keel, W., Masters, K. L., Mehta, V., Simmons, B. D., Smethurst, R., Smith, L., Baeten, E. M., & MacMillan, C. (2022). Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies. Monthly Notices of the Royal Astronomical Society, 509(3), 3966-3988. https://doi.org/10.1093/mnras/stab2093

Journal Article Type Article
Acceptance Date Jul 16, 2021
Online Publication Date Sep 30, 2021
Publication Date Jan 1, 2022
Deposit Date Jan 26, 2022
Publicly Available Date Jan 26, 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 509
Issue 3
Pages 3966-3988
DOI https://doi.org/10.1093/mnras/stab2093
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://nottingham-repository.worktribe.com/output/7340708
Publisher URL https://academic.oup.com/mnras/article/509/3/3966/6378289

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