Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model

The core mass of galaxy clusters is an important probe of structure formation. Here, we evaluate the use of a Single-Halo model (SHM) as an efficient method to estimate the strong lensing cluster core mass, testing it with ray-traced images from the `Outer Rim' simulation. Unlike detailed lens...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2021-02
Hauptverfasser:	Remolina González, J D, Sharon, K, N Li, Mahler, G, Bleem, L E, Gladders, M, Niemiec, A
Format:	Artikel
Sprache:	eng
Schlagworte:	Bias Correlation analysis Galactic clusters Inspection Lenses Mass distribution Physics - Cosmology and Nongalactic Astrophysics Red shift Scattering
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!