“Merger identification”的版本间差异
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==reference== |
==reference== |
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* Using transfer learning to detect galaxy mergers[https://ui.adsabs.harvard.edu/abs/2018MNRAS.479..415A/abstract] |
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* Deep learning predictions of galaxy merger stage and the importance of observational realism [https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.5390B/abstract] |
* Deep learning predictions of galaxy merger stage and the importance of observational realism [https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.5390B/abstract] |
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* Identification of low surface brightness tidal features in galaxies using convolutional neural networks [https://ui.adsabs.harvard.edu/abs/2019MNRAS.483.2968W/abstract] |
* Identification of low surface brightness tidal features in galaxies using convolutional neural networks [https://ui.adsabs.harvard.edu/abs/2019MNRAS.483.2968W/abstract] |
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2021年4月22日 (四) 14:27的版本
reference
- Using transfer learning to detect galaxy mergers[1]
- Deep learning predictions of galaxy merger stage and the importance of observational realism [2]
- Identification of low surface brightness tidal features in galaxies using convolutional neural networks [3]
- Identifying galaxy mergers in observations and simulations with deep learning[4]