Exploiting Machine Learning and Disequilibrium in Galaxy Clusters to Obtain a Mass Profile

We use 3D k -means clustering to characterize galaxy substructure in the A2146 cluster of galaxies ( z = 0.2343). This method objectively characterizes the cluster’s substructure using projected position and velocity data for 67 galaxies within a 2.305 Mpc circular region centered on the cluster...

書誌詳細
主要な著者:	Mark J. Henriksen, Prajwal Panda
フォーマット:	論文
言語:	English
出版事項:	IOP Publishing 2024-01-01
シリーズ:	The Astrophysical Journal Letters
主題:	Galaxy clusters Astroinformatics Large-scale structure of the universe Dark matter distribution
オンライン･アクセス:	https://doi.org/10.3847/2041-8213/ad1ede

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