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Practical galaxy morphology tools from deep supervised representation learning

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Practical galaxy morphology tools from deep supervised representation learning. / Walmsley, Mike; Scaife, Anna M M; Lintott, Chris et al.
In: Monthly Notices of the Royal Astronomical Society, 28.02.2022.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Walmsley, M, Scaife, AMM, Lintott, C, Lochner, M, Etsebeth, V, Géron, T, Dickinson, H, Fortson, L, Kruk, S, Masters, KL, Mantha, KB & Simmons, BD 2022, 'Practical galaxy morphology tools from deep supervised representation learning', Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stac525

APA

Walmsley, M., Scaife, A. M. M., Lintott, C., Lochner, M., Etsebeth, V., Géron, T., Dickinson, H., Fortson, L., Kruk, S., Masters, K. L., Mantha, K. B., & Simmons, B. D. (2022). Practical galaxy morphology tools from deep supervised representation learning. Monthly Notices of the Royal Astronomical Society. Advance online publication. https://doi.org/10.1093/mnras/stac525

Vancouver

Walmsley M, Scaife AMM, Lintott C, Lochner M, Etsebeth V, Géron T et al. Practical galaxy morphology tools from deep supervised representation learning. Monthly Notices of the Royal Astronomical Society. 2022 Feb 28. Epub 2022 Feb 28. doi: 10.1093/mnras/stac525

Author

Walmsley, Mike ; Scaife, Anna M M ; Lintott, Chris et al. / Practical galaxy morphology tools from deep supervised representation learning. In: Monthly Notices of the Royal Astronomical Society. 2022.

Bibtex

@article{c5b681cf14a040f090c62d43f6ab41af,
title = "Practical galaxy morphology tools from deep supervised representation learning",
abstract = "Astronomers have typically set out to solve supervised machine learning problems by creating their own representations from scratch. We show that deep learning models trained to answer every Galaxy Zoo DECaLS question learn meaningful semantic representations of galaxies that are useful for new tasks on which the models were never trained. We exploit these representations to outperform several recent approaches at practical tasks crucial for investigating large galaxy samples. The first task is identifying galaxies of similar morphology to a query galaxy. Given a single galaxy assigned a free text tag by humans (e.g. {\textquoteleft}#diffuse{\textquoteright}), we can find galaxies matching that tag for most tags. The second task is identifying the most interesting anomalies to a particular researcher. Our approach is 100 per cent accurate at identifying the most interesting 100 anomalies (as judged by Galaxy Zoo 2 volunteers). The third task is adapting a model to solve a new task using only a small number of newly-labelled galaxies. Models fine-tuned from our representation are better able to identify ring galaxies than models fine-tuned from terrestrial images (ImageNet) or trained from scratch. We solve each task with very few new labels; either one (for the similarity search) or several hundred (for anomaly detection or fine-tuning). This challenges the longstanding view that deep supervised methods require new large labelled datasets for practical use in astronomy. To help the community benefit from our pretrained models, we release our fine-tuning code zoobot. Zoobot is accessible to researchers with no prior experience in deep learning.",
keywords = "Space and Planetary Science, Astronomy and Astrophysics",
author = "Mike Walmsley and Scaife, {Anna M M} and Chris Lintott and Michelle Lochner and Verlon Etsebeth and Tobias G{\'e}ron and Hugh Dickinson and Lucy Fortson and Sandor Kruk and Masters, {Karen L} and Mantha, {Kameswara Bharadwaj} and Simmons, {Brooke D}",
year = "2022",
month = feb,
day = "28",
doi = "10.1093/mnras/stac525",
language = "English",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",

}

RIS

TY - JOUR

T1 - Practical galaxy morphology tools from deep supervised representation learning

AU - Walmsley, Mike

AU - Scaife, Anna M M

AU - Lintott, Chris

AU - Lochner, Michelle

AU - Etsebeth, Verlon

AU - Géron, Tobias

AU - Dickinson, Hugh

AU - Fortson, Lucy

AU - Kruk, Sandor

AU - Masters, Karen L

AU - Mantha, Kameswara Bharadwaj

AU - Simmons, Brooke D

PY - 2022/2/28

Y1 - 2022/2/28

N2 - Astronomers have typically set out to solve supervised machine learning problems by creating their own representations from scratch. We show that deep learning models trained to answer every Galaxy Zoo DECaLS question learn meaningful semantic representations of galaxies that are useful for new tasks on which the models were never trained. We exploit these representations to outperform several recent approaches at practical tasks crucial for investigating large galaxy samples. The first task is identifying galaxies of similar morphology to a query galaxy. Given a single galaxy assigned a free text tag by humans (e.g. ‘#diffuse’), we can find galaxies matching that tag for most tags. The second task is identifying the most interesting anomalies to a particular researcher. Our approach is 100 per cent accurate at identifying the most interesting 100 anomalies (as judged by Galaxy Zoo 2 volunteers). The third task is adapting a model to solve a new task using only a small number of newly-labelled galaxies. Models fine-tuned from our representation are better able to identify ring galaxies than models fine-tuned from terrestrial images (ImageNet) or trained from scratch. We solve each task with very few new labels; either one (for the similarity search) or several hundred (for anomaly detection or fine-tuning). This challenges the longstanding view that deep supervised methods require new large labelled datasets for practical use in astronomy. To help the community benefit from our pretrained models, we release our fine-tuning code zoobot. Zoobot is accessible to researchers with no prior experience in deep learning.

AB - Astronomers have typically set out to solve supervised machine learning problems by creating their own representations from scratch. We show that deep learning models trained to answer every Galaxy Zoo DECaLS question learn meaningful semantic representations of galaxies that are useful for new tasks on which the models were never trained. We exploit these representations to outperform several recent approaches at practical tasks crucial for investigating large galaxy samples. The first task is identifying galaxies of similar morphology to a query galaxy. Given a single galaxy assigned a free text tag by humans (e.g. ‘#diffuse’), we can find galaxies matching that tag for most tags. The second task is identifying the most interesting anomalies to a particular researcher. Our approach is 100 per cent accurate at identifying the most interesting 100 anomalies (as judged by Galaxy Zoo 2 volunteers). The third task is adapting a model to solve a new task using only a small number of newly-labelled galaxies. Models fine-tuned from our representation are better able to identify ring galaxies than models fine-tuned from terrestrial images (ImageNet) or trained from scratch. We solve each task with very few new labels; either one (for the similarity search) or several hundred (for anomaly detection or fine-tuning). This challenges the longstanding view that deep supervised methods require new large labelled datasets for practical use in astronomy. To help the community benefit from our pretrained models, we release our fine-tuning code zoobot. Zoobot is accessible to researchers with no prior experience in deep learning.

KW - Space and Planetary Science

KW - Astronomy and Astrophysics

U2 - 10.1093/mnras/stac525

DO - 10.1093/mnras/stac525

M3 - Journal article

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

ER -