Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/abb2a1/pdf
Reference122 articles.
1. The Dark Energy Survey: Data Release 1
2. Hubble Frontier Fields: systematic errors in strong lensing models of galaxy clusters – implications for cosmography
3. The 8 O'Clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data
4. Cosmological Parameters from Observations of Galaxy Clusters
5. Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
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1. COOL-LAMPS. VI. Lens Model and New Constraints on the Properties of COOL J1241+2219, a Bright z = 5 Lyman Break Galaxy and its z = 1 Cluster Lens;The Astrophysical Journal;2024-02-28
2. The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint;The Astrophysical Journal Supplement Series;2022-03-01
3. Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii;The Astrophysical Journal;2021-10-01
4. Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-halo Lens Model;The Astrophysical Journal;2021-04-01
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