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Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
Remolina Gonzalez, J. D.1; Sharon, K.1; Mahler, G.1,2,3; Fox, C.1; Garcia Diaz, C. A.4; Napier, K.1; Bleem, L. E.5,6; Gladders, M. D.6,7; Li, N.8,9; Niemiec, A.1,2,3
2021-10-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume920Issue:2Pages:14
AbstractThe core mass of galaxy clusters is both an important anchor of the radial mass distribution profile and a probe of structure formation. With thousands of strong lensing galaxy clusters being discovered by current and upcoming surveys, timely, efficient, and accurate core mass estimates are needed. We assess the results of two efficient methods to estimate the core mass of strong lensing clusters: the mass enclosed by the Einstein radius (M(
Funding OrganizationNASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics
DOI10.3847/1538-4357/ac16d8
WOS KeywordHUBBLE-FRONTIER-FIELDS ; GIANT ARCS ; NONPARAMETRIC INVERSION ; DARK-MATTER ; RELICS ; WEAK ; SPECTROSCOPY ; CONSTRAINTS ; PREDICTIONS ; CLASH
Language英语
Funding ProjectNASA[NAS5-26555] ; National Science Foundation Graduate Research Fellowship[DGE 1256260] ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant[MARACAS-DLV-896778] ; U.S. Department of Energy, Office of Science, Office of High Energy Physics[DE-AC02-06CH11357]
Funding OrganizationNASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; NASA ; NASA ; National Science Foundation Graduate Research Fellowship ; National Science Foundation Graduate Research Fellowship ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; European Union's Horizon 2020 research and innovation program under Marie Skodowska-Curie grant ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000709105900001
PublisherIOP Publishing Ltd
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/74423
Collection中国科学院国家天文台
Corresponding AuthorRemolina Gonzalez, J. D.
Affiliation1.Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA
2.Univ Durham, Dept Phys, Ctr Extragalact Astron, Durham DH1 3LE, England
3.Univ Durham, Inst Computat Cosmol, South Rd, Durham DH1 3LE, England
4.Delaware State Univ, Div Phys Engn Math & Comp Sci, 1200 N Dupont Hwy, Dover, DE USA
5.Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA
6.Univ Chicago, Kavli Inst Cosmol Phys, 5640 S Ellis Ave, Chicago, IL 60637 USA
7.Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
8.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, A20 Datun Rd, Beijing 100012, Peoples R China
9.Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England
Recommended Citation
GB/T 7714
Remolina Gonzalez, J. D.,Sharon, K.,Mahler, G.,et al. Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii[J]. ASTROPHYSICAL JOURNAL,2021,920(2):14.
APA Remolina Gonzalez, J. D..,Sharon, K..,Mahler, G..,Fox, C..,Garcia Diaz, C. A..,...&Niemiec, A..(2021).Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii.ASTROPHYSICAL JOURNAL,920(2),14.
MLA Remolina Gonzalez, J. D.,et al."Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii".ASTROPHYSICAL JOURNAL 920.2(2021):14.
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