Detailed Mass Map of CL 0024+1654 from Strong Lensing

Tyson, J. Anthony; Kochanski, Greg P.; Dell'Antonio, Ian P.

doi:10.1086/311314

Cited by 335Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesAstrophysical Phenomena and Observations

Detailed Mass Map of CL 0024+1654 from Strong Lensing

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Tyson, J. Anthony, Kochanski, Greg P., Dell'Antonio, Ian P.·1998·The Astrophysical Journal

DOI 10.1086/311314

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Abstract

We construct a high-resolution mass map of the z =0.39 cluster 0024+1654, based on a parametric inversion of the associated gravitational lens. The lens creates eight well-resolved subimages of a background galaxy, seen in deep imaging with the Hubble Space Telescope . Excluding mass concentrations centered on visible galaxies, more than 98% of the remaining mass is represented by a smooth concentration of dark matter centered near the brightest cluster galaxies, with a 35 h -1 kpc soft core. The asymmetry in the mass distribution is less than 3% inside 107 h -1 kpc radius. The dark matter distribution we observe in CL 0024 is far more smooth, symmetric, and nonsingular than in typical simulated clusters in either Ω=1 or Ω=0.3 cold dark matter cosmologies. Integrated to a 107 h -1 kpc radius, the rest-frame mass-to-light ratio is M / L V =276±40 h (M/L V ) ☉ .

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LSST will search for strong gravitational lenses to a faint surface brightness limit.
“Search for strong gravitational lenses to a faint surface brightness limit”
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Astrophysical Journal Letters, in press Detailed Mass Map of CL0024+1654 from Strong LensingPreprint
Tyson, J. A., Kochanski, G., & Dell’Antonio, I. (1998)
Self-citation
A Wide‐FieldHubble Space TelescopeStudy of the Cluster Cl 0024+1654 at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0.4$ \end{document} . II. The Cluster Mass Distribution
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Preprint typeset using L ATEX style emulateapj v. 26/01/00 A WIDE FIELD HUBBLE SPACE TELESCOPE STUDY OF THE CLUSTER CL0024+1654 AT Z = 0.4 II: THE CLUSTER MASS DISTRIBUTIONPreprint
Kneib, J., Hudelot, P., Ellis, R. S., Treu, T., Graham, P., Marshall, P. J., Czoske, O., Smail, I., & Natarajan, P. (2008)
Detailed Mass Distribution in CL0024 from Strong Lensing
Kochanski, G., Dell’Antonio, I., & Tyson, T. (1996) · American Astronomical Society Meeting Abstracts
Self-citation
On the Mass Profile of Galaxy Cluster C[CLC]l[/CLC] 0024+1654 Inferred from Strong Lensing
Shapiro, P. R., & Iliev, I. T. (2000) · The Astrophysical Journal · doi:10.1086/312919 · Cited by 29 · see citing works

Authors: Tyson, J. A., Kochanski, G. P., & Dell'Antonio, I. P.
Affiliations: Alcatel-Lucent (France) (FR)
Venue: The Astrophysical Journal
Publisher: American Astronomical Society
Published: 1998-05-10
Volume: 498
Issue: 2
Pages: L107-L110
ISSN: 0004-637X (ISSN-L)
DOI: 10.1086/311314
OpenAlex: W2053222792
Cited by: 335
References: 26
Citations by year: 2026: 3 · 2025: 10 · 2024: 10 · 2023: 4 · 2022: 6 · 2021: 5 · 2020: 6 · 2019: 10 · 2018: 9 · 2017: 8 · 2016: 10 · 2015: 3 · 2014: 11 · 2013: 8 · 2012: 13
FWCI: 18.23
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: The Astrophysical Journal (publishedVersion)
arXiv (Cornell University) (submittedVersion)
CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
arXiv (Cornell University)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
Keywords: galaxy clusters, dark matter distribution, strong gravitational lensing, mass maps, brightest cluster galaxies, soft core, mass-to-light ratio, cluster cosmology, cold dark matter simulations

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Detailed Mass Map of CL 0024+1654 from Strong Lensing

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