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Detailed Mass Map of CL 0024+1654 from Strong Lensing
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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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“Search for strong gravitational lenses to a faint surface brightness limit”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Tyson et al. 1998
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Metadata
- 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)
- 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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
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