Cited by 382Galaxies: Formation, Evolution, PhenomenaAdvanced Neural Network ApplicationsStellar, planetary, and galactic studies

Improving galaxy morphologies for SDSS with Deep Learning

Open access
Domínguez Sánchez, H, Huertas-Company, M, Bernardi, M, Tuccillo, D, Fischer, J L·2018·Monthly Notices of the Royal Astronomical Society

Abstract

We present a morphological catalogue for ∼670 000 galaxies in the Sloan Digital Sky Survey in two flavours: T-type, related to the Hubble sequence, and Galaxy Zoo 2 (GZ2 hereafter) classification scheme. By combining accurate existing visual classification catalogues with machine learning, we provide the largest and most accurate morphological catalogue up to date. The classifications are obtained with Deep Learning algorithms using Convolutional Neural Networks (CNNs). We use two visual classification catalogues, GZ2 and Nair & Abraham (2010), for training CNNs with colour images in order to obtain T-types and a series of GZ2 type questions (disc/features, edge-on galaxies, bar signature, bulge prominence, roundness, and mergers). We also provide an additional probability enabling a separation between pure elliptical (E) from S0, where the T-type model is not so efficient. For the T-type, our results show smaller offset and scatter than previous models trained with support vector machines. For the GZ2 type questions, our models have large accuracy (>97 per cent), precision and recall values (>90 per cent), when applied to a test sample with the same characteristics as the one used for training. The catalogue is publicly released with the paper.

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1093/mnras/sty338

Cites

43 of 43 references verified0 citation errors · 0 not checkable

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

Flagged first, then by citations

Research works printed but not linked: 6

  1. Barchi P. H., da Costa F. G., Sautter R., Moura T. C., Stalder D. H., Rosa R. R., de Carvalho R. R., 2017, preprint, ( arXiv:1705.06818 ) · arXiv
  2. Ciresan D., Meier U., Schmidhuber J., 2012, in Computer Vision and Pattern Recognition (CVPR), 2012 IEEE Conference on. pp 3642-3649
  3. Hinton G. E., Srivastava N., Krizhevsky A., Sutskever I., Salakhutdinov R., 2012, CoRR, abs/1207.0580 · arXiv
  4. Nair V., Hinton G. E., 2010, in F ˜ Aijrnkranz J., Joachims T., eds, Proceedings of the 27th International Conference on Machine Learning (ICML-10). Omnipress, pp 807-814, http://www. icml2010.org/papers/432.pdf
  5. Russakovsky O., et al., 2015, International Journal of Computer Vision (IJCV), 115, 211
  6. Srivastava N., Hinton G. E., Krizhevsky A., Sutskever I., Salakhutdinov R., 2014, Journal of Machine Learning Research, 15, 1929

Cited by

Sorted by citations

Authors
Domínguez Sánchez, H., Huertas-Company, M., Bernardi, M., Tuccillo, D., & Fischer, J. L.
Affiliations
  • Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA
  • Centre National de la Recherche Scientifique (FR)
Venue
Monthly Notices of the Royal Astronomical Society
Published
2018-02-09
Volume
476
Issue
3
Pages
3661-3676
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2768455873
Cited by
382
References
43
Citations by year
2026: 28 · 2025: 47 · 2024: 48 · 2023: 47 · 2022: 57 · 2021: 64 · 2020: 41 · 2019: 41 · 2018: 9
FWCI
20.80
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • HAL (submittedVersion, cc-by)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Computer Science › Computer Vision and Pattern Recognition › Advanced Neural Network Applications
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
galaxy morphology, convolutional neural networks, Galaxy Zoo 2, Hubble sequence, visual categorization, galactic bars, edge-on galaxies, mergers, S0 galaxies, elliptical galaxies, Sloan Digital Sky Survey, color images

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review