Galaxy Morphology Classification using Neural Ordinary Differential Equations
arXiv:2012.07735 · doi:10.1016/j.ascom.2021.100543
Abstract
We introduce a continuous depth version of the Residual Network (ResNet) called Neural ordinary differential equations (NODE) for the purpose of galaxy morphology classification. We carry out a classification of galaxy images from the Galaxy Zoo 2 dataset, consisting of five distinct classes, and obtained an accuracy between 91-95\%, depending on the image class. We train NODE with different numerical techniques such as adjoint and Adaptive Checkpoint Adjoint (ACA) and compare them against ResNet. While ResNet has certain drawbacks, such as time consuming architecture selection (e.g. the number of layers) and the requirement of a large dataset needed for training, NODE can overcome these limitations. Through our results, we show that that the accuracy of NODE is comparable to ResNet, and the number of parameters used is about one-third as compared to ResNet, thus leading to a smaller memory footprint, which would benefit next generation surveys.
10 pages, 5 figures. Now also used NODE_ACA. Accepted for publication in Astronomy and Computing
References in corpus (16)
- Very Deep Convolutional Networks for Large-Scale Image Recognition
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- Galaxy Zoo: the dependence of morphology and colour on environment
- Machine Learning in Astronomy: a practical overview
- Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS
- Galaxy Zoo: Morphological Classifications for 120,000 Galaxies in HST Legacy Imaging
- Galaxy morphological classification in deep-wide surveys via unsupervised machine learning
- ANODE: Unconditionally Accurate Memory-Efficient Gradients for Neural ODEs
- AstroVaDEr: Astronomical Variational Deep Embedder for Unsupervised Morphological Classification of Galaxies and Synthetic Image Generation
- Adaptive Checkpoint Adjoint Method for Gradient Estimation in Neural ODE
- Explaining deep learning of galaxy morphology with saliency mapping
- Galaxy classification: deep learning on the OTELO and COSMOS databases
- MRI Image Reconstruction via Learning Optimization Using Neural ODEs
- Neural ODE with Temporal Convolution and Time Delay Neural Networks for Small-Footprint Keyword Spotting
- Neural ODEs for Image Segmentation with Level Sets
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- Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks
- Galaxy Image Classification using Hierarchical Data Learning with Weighted Sampling and Label Smoothing
- Machine learning technique for morphological classification of galaxies from the SDSS. III. Image-based inference of detailed features
- Galaxy Morphological Classification with Efficient Vision Transformer