“Merger identification”的版本间差异

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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]
* 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]
* Identifying galaxy mergers in observations and simulations with deep learning[https://ui.adsabs.harvard.edu/abs/2019A%26A...626A..49P/abstract]

2021年4月22日 (四) 14:25的版本


reference

  • Deep learning predictions of galaxy merger stage and the importance of observational realism [1]
  • Identification of low surface brightness tidal features in galaxies using convolutional neural networks [2]
  • Identifying galaxy mergers in observations and simulations with deep learning[3]
取自“http://cluster.shao.ac.cn/wiki/index.php?title=Merger_identification&oldid=4138”