Journal article
Radio galaxy zoo: Unsupervised clustering of convolutionally auto-encoded radio-astronomical images
- Abstract:
- This paper demonstrates a novel and efficient unsupervised clustering method with the combination of a self-organizing 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 labeled 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 neighborhood similarity and K-means clustering of radio-astronomical features. 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) data set image features which can be applied to new radio survey data.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(Preview, Accepted manuscript, 8.5MB, Terms of use)
-
- Publisher copy:
- 10.1088/1538-3873/ab213d
Authors
- Publisher:
- IOP Publishing
- Journal:
- Publications of the Astronomical Society of the Pacific More from this journal
- Volume:
- 131
- Issue:
- 1004
- Article number:
- 108011
- Publication date:
- 2019-09-11
- Acceptance date:
- 2019-05-13
- DOI:
- EISSN:
-
1538-3873
- ISSN:
-
0004-6280
- Language:
-
English
- Keywords:
- Pubs id:
-
1011736
- Local pid:
-
pubs:1011736
- Deposit date:
-
2021-03-09
Terms of use
- Copyright holder:
- Astronomical Society of the Pacific
- Copyright date:
- 2019
- Rights statement:
- © 2019. The Astronomical Society of the Pacific. All rights reserved.
- Notes:
- This is the accepted manuscript version of the article. The final published version is available from IOP Publishing at https://doi.org/10.1088/1538-3873/ab213d
If you are the owner of this record, you can report an update to it here: Report update to this record