Radio Galaxy Zoo: Compact and extended radio source classification with deep learning
V. Lukic, M. Br\"uggen, J.K. Banfield, O.I. Wong, L. Rudnick, R.P., Norris, B. Simmons

TL;DR
This paper develops and tests a convolutional neural network to classify radio sources into compact and extended morphologies, achieving over 94% accuracy, aiding astronomical image analysis.
Contribution
It introduces a CNN architecture optimized for radio source morphology classification and evaluates factors affecting its performance, including data size and hyperparameters.
Findings
Achieved 97.4% accuracy in binary classification of radio source morphology.
Extended to four classes with 93.5% accuracy, final test accuracy of 94.8%.
Sigma clipping offers limited benefit except with small training datasets.
Abstract
Machine learning techniques have been increasingly useful in astronomical applications over the last few years, for example in the morphological classification of galaxies. Convolutional neural networks have proven to be highly effective in classifying objects in image data. The current work aims to establish when multiple components are present, in the astronomical context of synthesis imaging observations of radio sources. To this effect, we design a convolutional neural network to differentiate between different morphology classes using sources from the Radio Galaxy Zoo (RGZ) citizen science project. In this first step, we focus on exploring the factors that affect the performance of such neural networks, such as the amount of training data, number and nature of layers and the hyperparameters. We begin with a simple experiment in which we only differentiate between two extreme…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
