4.3 Article

Classifying Galaxy Morphologies with Few-shot Learning

Journal

RESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume 22, Issue 5, Pages -

Publisher

NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
DOI: 10.1088/1674-4527/ac5732

Keywords

Galaxies; Galaxy; morphological classification; Method; neural networks

Funding

  1. China Manned Space Project [CMS-CSST-2021-A01]
  2. Jiangsu Key Laboratory of Big Data Security and Intelligent Processing

Ask authors/readers for more resources

The taxonomy of galaxy morphology is critical in astrophysics, and few-shot learning, a machine learning method, is effective in addressing the challenges faced by traditional methods and supervised deep learning, offering high accuracy and automation.
The taxonomy of galaxy morphology is critical in astrophysics as the morphological properties are powerful tracers of galaxy evolution. With the upcoming Large-scale Imaging Surveys, billions of galaxy images challenge astronomers to accomplish the classification task by applying traditional methods or human inspection. Consequently, machine learning, in particular supervised deep learning, has been widely employed to classify galaxy morphologies recently due to its exceptional automation, efficiency, and accuracy. However, supervised deep learning requires extensive training sets, which causes considerable workloads; also, the results are strongly dependent on the characteristics of training sets, which leads to biased outcomes potentially. In this study, we attempt Few-shot Learning to bypass the two issues. Our research adopts the data set from the Galaxy Zoo Challenge Project on Kaggle, and we divide it into five categories according to the corresponding truth table. By classifying the above data set utilizing few-shot learning based on Siamese Networks and supervised deep learning based on AlexNet, VGG_16, and ResNet_50 trained with different volumes of training sets separately, we find that few-shot learning achieves the highest accuracy in most cases, and the most significant improvement is 21% compared to AlexNet when the training sets contain 1000 images. In addition, to guarantee the accuracy is no less than 90%, few-shot learning needs similar to 6300 images for training, while ResNet_50 requires similar to 13,000 images. Considering the advantages stated above, foreseeably, few-shot learning is suitable for the taxonomy of galaxy morphology and even for identifying rare astrophysical objects, despite limited training sets consisting of observational data only.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.3
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Astronomy & Astrophysics

Optimizing automatic morphological classification of galaxies with machine learning and deep learning using Dark Energy Survey imaging

Ting-Yun Cheng, Christopher J. Conselice, Alfonso Aragon-Salamanca, Nan Li, Asa F. L. Bluck, Will G. Hartley, James Annis, David Brooks, Peter Doel, Juan Garcia-Bellido, David J. James, Kyler Kuehn, Nikolay Kuropatkin, Mathew Smith, Flavia Sobreira, Gregory Tarle

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

Identifying strong lenses with unsupervised machine learning using convolutional autoencoder

Ting-Yun Cheng, Nan Li, Christopher J. Conselice, Alfonso Aragon-Salamanca, Simon Dye, Robert B. Metcalf

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

The LSST DESC DC2 Simulated Sky Survey

Bela Abolfathi, David Alonso, Robert Armstrong, Eric Aubourg, Humna Awan, Yadu N. Babuji, Franz Erik Bauer, Rachel Bean, George Beckett, Rahul Biswas, Joanne R. Bogart, Dominique Boutigny, Kyle Chard, James Chiang, Chuck F. Claver, Johann Cohen-Tanugi, Celine Combet, Andrew J. Connolly, Scott F. Daniel, Seth W. Digel, Alex Drlica-Wagner, Richard Dubois, Emmanuel Gangler, Eric Gawiser, Thomas Glanzman, Phillipe Gris, Salman Habib, Andrew P. Hearin, Katrin Heitmann, Fabio Hernandez, Renee Hlozek, Joseph Hollowed, Mustapha Ishak, Zeljko Ivezic, Mike Jarvis, Saurabh W. Jha, Steven M. Kahn, J. Bryce Kalmbach, Heather M. Kelly, Eve Kovacs, Danila Korytov, K. Simon Krughoff, Craig S. Lage, Francois Lanusse, Patricia Larsen, Laurent Le Guillou, Nan Li, Emily Phillips Longley, Robert H. Lupton, Rachel Mandelbaum, Yao-Yuan Mao, Phil Marshall, Joshua E. Meyers, Marc Moniez, Christopher B. Morrison, Andrei Nomerotski, Paul O'Connor, HyeYun Park, Ji Won Park, Julien Peloton, Daniel Perrefort, James Perry, Stephane Plaszczynski, Adrian Pope, Andrew Rasmussen, Kevin Reil, Aaron J. Roodman, Eli S. Rykoff, F. Javier Sanchez, Samuel J. Schmidt, Daniel Scolnic, Christopher W. Stubbs, J. Anthony Tyson, Thomas D. Uram, Antonio Villarreal, Christopher W. Walter, Matthew P. Wiesner, W. Michael Wood-Vasey, Joe Zuntz

Summary: The simulated sky survey for the second data challenge (DC2) serves as preparation for the analysis of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) by the LSST Dark Energy Science Collaboration (LSST DESC). This modeling effort emphasizes interconnectivity across multiple science domains in a way that has not been tried before, covering a wide range of aspects from N-body simulation to image processing with LSST-like observations. The DC2 sky survey allows LSST DESC to develop analysis pipelines, test image processing software, and explore new scientific ideas in both static and time domain cosmology.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2021)

Article Astronomy & Astrophysics

Auto-identification of unphysical source reconstructions in strong gravitational lens modelling

Jacob Maresca, Simon Dye, Nan Li

Summary: This study examines a method using a Convolutional Neural Network to analyze lens modeling and source reconstruction, showcasing a significant reduction in unphysical source reconstructions by reinitializing the models based on CNN predictions.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-halo Lens Model

J. D. Remolina Gonzalez, K. Sharon, N. Li, G. Mahler, L. E. Bleem, M. Gladders, A. Niemiec

Summary: The study evaluated the use of a single-halo model as an efficient method to estimate the strong lensing cluster core mass, finding that the projected core mass estimated with this method has a small scatter and bias compared to the true mass. Excluding models that fail visual inspection test can reduce the bias and scatter, while excluding single giant arc configurations can improve the accuracy of the model predictions. When the source redshift is unknown, the model-predicted redshifts are overestimated, underlining the importance of securing spectroscopic redshifts of background sources.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

The impact of line-of-sight structures on measuring H0 with strong lensing time delays

Nan Li, Christoph Becker, Simon Dye

Summary: This paper investigates the impact of line-of-sight structures on time-delay measurements in strong lensing systems and concludes that lens modelling must incorporate multiple-lens planes to accurately infer H-0.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting

James Pearson, Jacob Maresca, Nan Li, Simon Dye

Summary: The study trains a CNN to predict mass profile parameters of galaxy-galaxy gravitational lenses, with significantly lower errors compared to traditional methods, especially when incorporating uncertainties predicted by the CNN. Combining neural networks with conventional techniques can greatly improve accuracy and speed in automated modelling.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii

J. D. Remolina Gonzalez, K. Sharon, G. Mahler, C. Fox, C. A. Garcia Diaz, K. Napier, L. E. Bleem, M. D. Gladders, N. Li, A. Niemiec

Summary: The core mass of galaxy clusters plays a crucial role in studying their structure formation. Efficient methods for estimating core mass are essential with the discovery of numerous strong lensing galaxy clusters. Advancements in observational techniques have improved the accuracy and depth of research on core mass in these clusters.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Identifying Outliers in Astronomical Images with Unsupervised Machine Learning

Yang Han, Zhiqiang Zou, Nan Li, Yanli Chen

Summary: Studying astronomical outliers is crucial for discovering previously unknown knowledge. However, mining rare and unexpected targets from vast amounts of data is a significant challenge. In this study, unsupervised machine learning approaches were used to identify outliers in galaxy image data, leading to promising results.

RESEARCH IN ASTRONOMY AND ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

The Quasar Candidate Catalogs of DESI Legacy Imaging Survey Data Release 9

Zizhao He, Nan Li

Summary: This study uses a machine learning algorithm to create a catalog of quasar candidates based on photometric data, providing priors for further object classification with spectroscopic data in the future. The catalog significantly reduces the workload for confirming quasars while maintaining high completeness.

RESEARCH IN ASTRONOMY AND ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

Detection of Strongly Lensed Arcs in Galaxy Clusters with Transformers

Peng Jia, Ruiqi Sun, Nan Li, Yu Song, Runyu Ning, Hongyan Wei, Rui Luo

Summary: Strong lensing in galaxy clusters allows us to study dense cores of dark matter halos, explore the distant universe, and test cosmological models. We propose a framework using a transformer-based detection algorithm and image simulation to detect cluster-scale strongly lensed arcs. Our approach achieves high accuracy, recall, and precision rates in simulated images and can detect most strongly lensed arcs in real observation images. We plan to apply our approach to available observations and simulated data from upcoming large-scale sky surveys for further testing and validation.

ASTRONOMICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Unsupervised Galaxy Morphological Visual Representation with Deep Contrastive Learning

Shoulin Wei, Yadi Li, Wei Lu, Nan Li, Bo Liang, Wei Dai, Zhijian Zhang

Summary: This paper proposes an approach based on contrastive learning to learn the visual representation of galaxy morphology using unlabeled data. By combining vision transformers and convolutional networks for feature extraction and fusion, rich semantic representation is provided. Experimental results show high accuracy in galaxy morphology classification and transferability and generalization ability of the proposed method.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2022)

Article Astronomy & Astrophysics

Discovering strongly lensed quasar candidates with catalogue-based methods from DESI Legacy Surveys

Zizhao He, Nan Li, Xiaoyue Cao, Rui Li, Hu Zou, Simon Dye

Summary: To better understand the origin of the Hubble tension, independent techniques like strong lensing time delays are needed. This study identified 620 new candidate multiply imaged lensed quasars within the DESI dataset, which will be further validated using spectroscopic and photometric data.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius

J. D. Remolina Gonzalez, K. Sharon, B. Reed, N. Li, G. Mahler, L. E. Bleem, M. Gladders, A. Niemiec, A. Acebron, H. Child

ASTROPHYSICAL JOURNAL (2020)

No Data Available