Transfer learning for radio galaxy classification

H. Tang*, A. M.M. Scaife, J. P. Leahy

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

49 Citations (Scopus)

Abstract

In the context of radio galaxy classification, most state-of-the-art neural network algorithms have been focused on single survey data. The question of whether these trained algorithms have cross-survey identification ability or can be adapted to develop classification networks for future surveys is still unclear. One possible solution to address this issue is transfer learning, which reuses elements of existing machine learning models for different applications. Here we present radio galaxy classification based on a 13-layer Deep Convolutional Neural Network (DCNN) using transfer learning methods between different radio surveys. We find that our machine learning models trained from a random initialization achieve accuracies comparable to those found elsewhere in the literature. When using transfer learning methods, we find that inheriting model weights pre-trained on FIRST images can boost model performance when retraining on lower resolution NVSS data, but that inheriting pre-trained model weights from NVSS and retraining on FIRST data impairs the performance of the classifier. We consider the implication of these results in the context of future radio surveys planned for next-generation radio telescopes such as ASKAP, MeerKAT, and SKA1-MID.

Original languageEnglish
Pages (from-to)3358-3375
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume488
Issue number3
DOIs
Publication statusPublished - 2019
Externally publishedYes

Keywords

  • Methods: statistical
  • Radio continuum: galaxies
  • Surveys

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