Galaxy Cluster Mass Estimation through the Splashback Radius

We present an analysis of the splashback radius ( R _sp ) and the associated splashback mass ( M _sp ) for a sample of galaxy clusters using Sloan Digital Sky Survey spectroscopic data and mock simulations. R _sp marks a physical boundary between the virialized core and the outer infall regions of c...

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Bibliographic Details
Main Authors: Lucas Gabriel-Silva, Laerte Sodré Jr.
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ade308
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