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Galaxy Zoo: Reproducing galaxy morphologies via machine learning

Galaxy Zoo: Reproducing galaxy morphologies via machine learning
Galaxy Zoo: Reproducing galaxy morphologies via machine learning
We present morphological classifications obtained using machine learning for objects in the Sloan Digital Sky Survey DR6 that have been classified by Galaxy Zoo into three classes, namely early types, spirals and point sources/artefacts. An artificial neural network is trained on a subset of objects classified by the human eye, and we test whether the machine-learning algorithm can reproduce the human classifications for the rest of the sample. We find that the success of the neural network in matching the human classifications depends crucially on the set of input parameters chosen for the machine-learning algorithm. The colours and parameters associated with profile fitting are reasonable in separating the objects into three classes. However, these results are considerably improved when adding adaptive shape parameters as well as concentration and texture. The adaptive moments, concentration and texture parameters alone cannot distinguish between early type galaxies and the point sources/artefacts. Using a set of 12 parameters, the neural network is able to reproduce the human classifications to better than 90 per cent for all three morphological classes. We find that using a training set that is incomplete in magnitude does not degrade our results given our particular choice of the input parameters to the network. We conclude that it is promising to use machine-learning algorithms to perform morphological classification for the next generation of wide-field imaging surveys and that the Galaxy Zoo catalogue provides an invaluable training set for such purposes.
1365-2966
342-353
Banerji, M.
ce0a04bf-70a4-4b64-9027-b1a01def7325
Lahav, O.
63be85ca-8350-4ccb-8e4f-efc74baf0198
Lintott, C.J.
e4b04dc5-8fe8-4f8a-b163-a1b2884c38fe
Abdalla, F.B.
b32ec665-df5e-4703-9eef-a9b15ea7cf08
Schawinski, K.
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Bamford, S.P.
3e492e0d-2002-488b-895e-4347a7b0d975
Andreescu, D.
2c228248-9665-4db4-ac59-245b582d4b26
Murray, P.
39a4779e-0ab5-41e1-8fa1-ab50ba92b7d3
Raddick, M.J.
6b100220-5c0c-4f22-8435-309316e7076a
Slosar, A.
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Szalay, A.
dfa901d5-f8f1-4eeb-8fb3-91d71ddf7ccf
Thomas, D.
e551e366-9e8c-48db-84bd-c16cc7af6401
Vandenberg, J.
553a97be-ddb4-4ced-b90c-bf620a8c205b
Banerji, M.
ce0a04bf-70a4-4b64-9027-b1a01def7325
Lahav, O.
63be85ca-8350-4ccb-8e4f-efc74baf0198
Lintott, C.J.
e4b04dc5-8fe8-4f8a-b163-a1b2884c38fe
Abdalla, F.B.
b32ec665-df5e-4703-9eef-a9b15ea7cf08
Schawinski, K.
b0386c64-6483-40ab-8537-13e3b0dcde48
Bamford, S.P.
3e492e0d-2002-488b-895e-4347a7b0d975
Andreescu, D.
2c228248-9665-4db4-ac59-245b582d4b26
Murray, P.
39a4779e-0ab5-41e1-8fa1-ab50ba92b7d3
Raddick, M.J.
6b100220-5c0c-4f22-8435-309316e7076a
Slosar, A.
86f91640-1935-4195-8387-99387fc9a145
Szalay, A.
dfa901d5-f8f1-4eeb-8fb3-91d71ddf7ccf
Thomas, D.
e551e366-9e8c-48db-84bd-c16cc7af6401
Vandenberg, J.
553a97be-ddb4-4ced-b90c-bf620a8c205b

Banerji, M., Lahav, O., Lintott, C.J., Abdalla, F.B., Schawinski, K., Bamford, S.P., Andreescu, D., Murray, P., Raddick, M.J., Slosar, A., Szalay, A., Thomas, D. and Vandenberg, J. (2010) Galaxy Zoo: Reproducing galaxy morphologies via machine learning. Monthly Notices Of The Royal Astronomical Society, 406 (1), 342-353. (doi:10.1111/j.1365-2966.2010.16713.x).

Record type: Article

Abstract

We present morphological classifications obtained using machine learning for objects in the Sloan Digital Sky Survey DR6 that have been classified by Galaxy Zoo into three classes, namely early types, spirals and point sources/artefacts. An artificial neural network is trained on a subset of objects classified by the human eye, and we test whether the machine-learning algorithm can reproduce the human classifications for the rest of the sample. We find that the success of the neural network in matching the human classifications depends crucially on the set of input parameters chosen for the machine-learning algorithm. The colours and parameters associated with profile fitting are reasonable in separating the objects into three classes. However, these results are considerably improved when adding adaptive shape parameters as well as concentration and texture. The adaptive moments, concentration and texture parameters alone cannot distinguish between early type galaxies and the point sources/artefacts. Using a set of 12 parameters, the neural network is able to reproduce the human classifications to better than 90 per cent for all three morphological classes. We find that using a training set that is incomplete in magnitude does not degrade our results given our particular choice of the input parameters to the network. We conclude that it is promising to use machine-learning algorithms to perform morphological classification for the next generation of wide-field imaging surveys and that the Galaxy Zoo catalogue provides an invaluable training set for such purposes.

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More information

Accepted/In Press date: 17 March 2010
Published date: 21 July 2010

Identifiers

Local EPrints ID: 500029
URI: http://eprints.soton.ac.uk/id/eprint/500029
ISSN: 1365-2966
PURE UUID: 538d8908-e094-460b-baf1-249ee85f10ad
ORCID for M. Banerji: ORCID iD orcid.org/0000-0002-0639-5141

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Date deposited: 11 Apr 2025 16:47
Last modified: 12 Apr 2025 02:03

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Contributors

Author: M. Banerji ORCID iD
Author: O. Lahav
Author: C.J. Lintott
Author: F.B. Abdalla
Author: K. Schawinski
Author: S.P. Bamford
Author: D. Andreescu
Author: P. Murray
Author: M.J. Raddick
Author: A. Slosar
Author: A. Szalay
Author: D. Thomas
Author: J. Vandenberg

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