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Radio Galaxy Zoo: Unsupervised Clustering of Convolutionally Auto-encoded Radio-astronomical Images

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arxiv 1906.02864 v1 pith:K42ULGS4 submitted 2019-06-07 astro-ph.IM cs.LG

classification astro-ph.IMcs.LG
keywords dataclusteringfeaturesmethodradioradio-astronomicaltrainingunsupervised
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This paper demonstrates a novel and efficient unsupervised clustering method with the combination of a Self-Organising Map (SOM) and a convolutional autoencoder. The rapidly increasing volume of radio-astronomical data has increased demand for machine learning methods as solutions to classification and outlier detection. Major astronomical discoveries are unplanned and found in the unexpected, making unsupervised machine learning highly desirable by operating without assumptions and labelled training data. Our approach shows SOM training time is drastically reduced and high-level features can be clustered by training on auto-encoded feature vectors instead of raw images. Our results demonstrate this method is capable of accurately separating outliers on a SOM with neighbourhood similarity and K-means clustering of radio-astronomical features complexity. We present this method as a powerful new approach to data exploration by providing a detailed understanding of the morphology and relationships of Radio Galaxy Zoo (RGZ) dataset image features which can be applied to new radio survey data.

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Cited by 1 Pith paper

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  1. How to Find Variable Active Galactic Nuclei with Machine Learning

    astro-ph.IM 2019-08 conditional novelty 4.0 of 10

    Self-organizing maps applied to nonparametric variability estimators identify variable AGN light curves with 86% purity and 66% completeness, comparable to deep learning.

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