Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii-Reference-Cited by-同舟云学术

Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii

Published:2021-10-01 Issue:2 Volume:920 Page:98
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Remolina González J. D.^ORCID,Sharon K.^ORCID,Mahler G.^ORCID,Fox C.^ORCID,Garcia Diaz C. A.,Napier K.^ORCID,Bleem L. E.^ORCID,Gladders M. D.^ORCID,Li N.^ORCID,Niemiec A.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac16d8/pdf

Reference133 articles.

1. RELICS: High-resolution Constraints on the Inner Mass Distribution of the z = 0.83 Merging Cluster RXJ0152.7-1357 from Strong Lensing

2. RELICS: Strong-lensing Analysis of the Massive Clusters MACS J0308.9+2645 and PLCK G171.9−40.7

3. Hubble Frontier Fields: systematic errors in strong lensing models of galaxy clusters – implications for cosmography

4. RELICS: A Very Large (θ E ∼ 40″) Cluster Lens—RXC J0032.1+1808

5. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

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