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Cited by 860

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Mapping the dark matter with weak gravitational lensing

Kaiser, Nick, Squires, Gordon·1993·The Astrophysical Journal

Abstract

We consider the problem of reconstructing the projected mass distribution in clusters from coherent distortions of background galaxies. The ellipticity of a background galaxy provides an estimate of the trace-free components of the tidal field {second partial derivative of {PHI} with respect to θ_i_, θ_j_} where {PHI}(θ) is the two-dimensional potential generated by the surface density {SIGMA}(θ). We present a technique for inverting this problem. The resulting surface density contains a strong, but incoherent, random component arising from the random intrinsic galaxy ellipticities. This can be removed by filtering. Our method is very similar in form to that of Tyson et al., and the latter is given a rigorous interpretation as a particular implementation of filtering. We present simulations to illustrate the application of the method.

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Metadata

Authors
Kaiser, N., & Squires, G.
Venue
The Astrophysical Journal
Published
1993-02
Volume
404
Pages
441
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2057504741
Cited by
860
References
0
FWCI
24.57
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Mapping the dark matter with weak gravitational lensing. https://app.cochat.ai/papers/10.1086/172297
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Kaiser, N., & Squires, G. (1993). Mapping the dark matter with weak gravitational lensing. The Astrophysical Journal. https://doi.org/10.1086/172297

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.