Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - Monthly notices of the royal …, 2015 - academic.oup.com
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …
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[引用][C] Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - Monthly Notices of the Royal …, 2015 - cir.nii.ac.jp
Rotation-invariant convolutional neural networks for galaxy morphology prediction | CiNii
Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 …

Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett… - Monthly Notices of the …, 2015 - ui.adsabs.harvard.edu
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …

[引用][C] Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - Mon. Not. R. Astron. Soc, 2015 - philpapers.org
Sander Dieleman, Kyle W. Willett & Joni Dambre, Rotation-invariant convolutional neural
networks for galaxy morphology prediction - PhilPapers Sign in | Create an account PhilPapers …
[PDF] academia.edu

[PDF][PDF] Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - academia.edu
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey (SDSS) have …

Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, K Willett, J Dambre - MONTHLY NOTICES OF THE …, 2015 - biblio.ugent.be
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …

Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - Monthly Notices of the Royal …, 2015 - experts.umn.edu
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …

Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - arXiv preprint arXiv:1503.07077, 2015 - arxiv.org
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey (SDSS) have …

Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett… - Monthly Notices of the …, 2015 - ieeexplore.ieee.org
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …
[PDF] researchgate.net

[PDF][PDF] Rotation-invariant convolutional neural networks for galaxy morphology prediction

S Dieleman, KW Willett, J Dambre - researchgate.net
Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey (SDSS) have …