Difference between revisions of "Merger identification"
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==reference== | ==reference== | ||
* Using transfer learning to detect galaxy mergers[https://ui.adsabs.harvard.edu/abs/2018MNRAS.479..415A/abstract] | |||
* 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] | * Identifying galaxy mergers in observations and simulations with deep learning[https://ui.adsabs.harvard.edu/abs/2019A%26A...626A..49P/abstract] | ||
Revision as of 14:27, 22 April 2021
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]