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Titlebook: Machine Learning for Astrophysics; Proceedings of the M Filomena Bufano,Simone Riggi,Francesco Schilliro Conference proceedings 2023 The Ed

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書目名稱Machine Learning for Astrophysics
副標(biāo)題Proceedings of the M
編輯Filomena Bufano,Simone Riggi,Francesco Schilliro
視頻videohttp://file.papertrans.cn/621/620583/620583.mp4
概述Provides a comprehensive view of machine learning techniques applied to astrophysics.Discusses limitations of ML applications to astrophysics.With a feature on how to face future radioastronomy data d
叢書名稱Astrophysics and Space Science Proceedings
圖書封面Titlebook: Machine Learning for Astrophysics; Proceedings of the M Filomena Bufano,Simone Riggi,Francesco Schilliro Conference proceedings 2023 The Ed
描述.This book reviews the state of the art in the exploitation of machine learning techniques for the astrophysics community and gives the reader a complete overview of the field. The contributed chapters allow the reader to easily digest the material through balanced theoretical and numerical methods and tools with applications in different fields of theoretical and observational astronomy. The book helps the reader to really understand and quantify both the opportunities and limitations of using machine learning in several fields of astrophysics..
出版日期Conference proceedings 2023
關(guān)鍵詞time series in astronomy and astrophysics; anomaly discovery in data; machine learning techniques; soft
版次1
doihttps://doi.org/10.1007/978-3-031-34167-0
isbn_softcover978-3-031-34169-4
isbn_ebook978-3-031-34167-0Series ISSN 1570-6591 Series E-ISSN 1570-6605
issn_series 1570-6591
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl
The information of publication is updating

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Machine Learning for Astrophysics978-3-031-34167-0Series ISSN 1570-6591 Series E-ISSN 1570-6605
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Classification of Evolved Stars with (Unsupervised) Machine Learning,wavelength photometric measurements. The foundation is a custom made reference dataset compiled from available stellar catalogues for target sources—AGB, Wolf Rayet, luminous blue variable and red supergiant stars. Our results indicate that applying HDBSCAN to UMAP’s feature representation seems to be the most effective approach for this usecase.
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Event Reconstruction for Neutrino Telescopes,ance to many physics analyses and searches, and improvements in both accuracy and speed have a direct, positive impact on the science. This proceeding will shortly review some common reconstruction methods, and present a few novel event reconstruction algorithms based on machine learning.
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