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

González, J.D. Remolina; Sharon, K.; Li, N.; Mahler, G.; Bleem, L.E.; Gladders, M.; Niemiec, A.

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


Authors

J.D. Remolina González

K. Sharon

N. Li

L.E. Bleem

M. Gladders

A. Niemiec



Abstract

The core mass of galaxy clusters is an important probe of structure formation. Here we evaluate the use of a singlehalo 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 models, the SHM represents the cluster mass distribution with a single halo and can be automatically generated from the measured lensing constraints. We find that the projected core mass estimated with this method, MSHM, has a scatter of 8.52% and a bias of 0.90% compared to the “true” mass within the same aperture. Our analysis shows no systematic correlation between the scatter or bias and the lens-source system properties. The bias and scatter can be reduced to 3.26% and 0.34%, respectively, by excluding models that fail a visual inspection test. We find that the SHM success depends on the lensing geometry, with single giant arc configurations accounting for most of the failed cases due to their limiting constraining power. When excluding such cases, we measure a scatter and bias of 3.88% and 0.84%, respectively. Finally, we find that when the source redshift is unknown, the model-predicted redshifts are overestimated, and the MSHM is underestimated by a few percent, highlighting the importance of securing spectroscopic redshifts of background sources. Our analysis provides a quantitative characterization of MSHM, enabling its efficient use as a tool to estimate the strong lensing cluster core masses in the large samples, expected from current and future surveys.

Journal Article Type Article
Acceptance Date Feb 11, 2021
Online Publication Date Apr 6, 2021
Publication Date 2021-04
Deposit Date Jan 11, 2022
Publicly Available Date Jan 13, 2022
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 910
Issue 2
Article Number 146
DOI https://doi.org/10.3847/1538-4357/abe62a
Public URL https://durham-repository.worktribe.com/output/1218804

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© 2021. The American Astronomical Society. All rights reserved






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