4.7 Article

Automatic morphological classification of galaxy images

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 399, Issue 3, Pages 1367-1372

Publisher

OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2009.15366.x

Keywords

methods: data analysis; techniques: image processing

Funding

  1. Intramural Research Program of the NIH
  2. National Institute on Aging
  3. Alfred P. Sloan Foundation
  4. National Science Foundation
  5. US Department of Energy
  6. National Aeronautics and Space Administration
  7. Japanese Monbukagakusho
  8. Max Planck Society
  9. Higher Education Funding Council for England

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We describe an image analysis supervised learning algorithm that can automatically classify galaxy images. The algorithm is first trained using manually classified images of elliptical, spiral and edge-on galaxies. A large set of image features is extracted from each image, and the most informative features are selected using Fisher scores. Test images can then be classified using a simple Weighted Nearest Neighbour rule such that the Fisher scores are used as the feature weights. Experimental results show that galaxy images from Galaxy Zoo can be classified automatically to spiral, elliptical and edge-on galaxies with an accuracy of similar to 90 per cent compared to classifications carried out by the author. Full compilable source code of the algorithm is available for free download, and its general-purpose nature makes it suitable for other uses that involve automatic image analysis of celestial objects.

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