Classifying Galaxy Morphologies with Few-Shot Learning
arXiv:2202.08172 · doi:10.1088/1674-4527/ac5732
Abstract
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 dataset from Galaxy Zoo Challenge Project on Kaggle, and we divide it into five categories according to the corresponding truth table. By classifying the above dataset 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 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 6300 images for training, while ResNet_50 requires 13000 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.
References in corpus (18)
- Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
- The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
- The Dark Energy Camera
- The Relationship Between Stellar Light Distributions of Galaxies and their Formation Histories
- A New Non-Parametric Approach to Galaxy Morphological Classification
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- Galaxy Zoo 2: detailed morphological classifications for 304,122 galaxies from the Sloan Digital Sky Survey
- A Catalog of Detailed Visual Morphological Classifications for 14034 Galaxies in the Sloan Digital Sky Survey
- A New Approach to Galaxy Morphology: I. Analysis of the Sloan Digital Sky Survey Early Data Release
- The EFIGI catalogue of 4458 nearby galaxies with detailed morphology
- The Physical Nature of Rest-UV Galaxy Morphology During the Peak Epoch of Galaxy Formation
- A Catalogue of Morphologically Classified Galaxies from the Sloan Digital Sky Survey: North Equatorial Region
- Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias
- Galaxy Morphology Classification with Deep Convolutional Neural Networks
- AUTOMATED MORPHOLOGICAL CLASSIFICATION OF APM GALAXIES BY SUPERVISED ARTIFICIAL NEURAL NETWORKS
- Optimising Automatic Morphological Classification of Galaxies with Machine Learning and Deep Learning using Dark Energy Survey Imaging
- Beyond the Hubble Sequence -- Exploring Galaxy Morphology with Unsupervised Machine Learning
- Galaxy Morphology Classification using Neural Ordinary Differential Equations
Cited by in corpus (6)
- Unsupervised Galaxy Morphological Visual Representation with Deep Contrastive Learning
- Identifying outliers in astronomical images with unsupervised machine learning
- Galaxy Morphology Classification Using Multi-Scale Convolution Capsule Network
- Galaxy Image Classification using Hierarchical Data Learning with Weighted Sampling and Label Smoothing
- Uncovering Tidal Treasures: Automated Classification of Faint Tidal Features in DECaLS Data
- Neural style transfer of weak lensing mass maps