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...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй
Үндсэн зохиолчид:	Mark J. Henriksen, Prajwal Panda
Формат:	Өгүүллэг
Хэл сонгох:	English
Хэвлэсэн:	IOP Publishing 2024-01-01
Цуврал:	The Astrophysical Journal Letters
Нөхцлүүд:	Galaxy clusters Astroinformatics Large-scale structure of the universe Dark matter distribution
Онлайн хандалт:	https://doi.org/10.3847/2041-8213/ad1ede

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