Galaxy-galaxy Lensing
Galaxy-Galaxy Lensing is a weak gravitational lensing phenomenon in which the gravitational field of a foreground galaxy distorts the images of background galaxies, enabling the measurement of the mass distribution of the foreground galaxy through statistical analysis of the induced shear.
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2017–2026
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Rachel Mandelbaum, Uroš Seljak, Guinevere Kauffmann et al. · Monthly Notices of the Royal Astronomical Society · 2006 · 719 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Princeton University
Princeton, United States
51 h-index
183 publications
19.1K citations
University of Chicago
Chicago, United States
43 h-index
241 publications
18.5K citations
The University of Tokyo
Tokyo, Japan
41 h-index
137 publications
9.6K citations
University of Arizona
Tucson, United States
39 h-index
97 publications
7.6K citations
Kavli Institute for Particle Astrophysics and Cosmology
Menlo Park, United States
38 h-index
191 publications
14.8K citations
University of California, Berkeley
Berkeley, United States
36 h-index
83 publications
6.9K citations
California Institute of Technology
Pasadena, United States
36 h-index
88 publications
7.3K citations

University of Edinburgh
Edinburgh, United Kingdom
35 h-index
123 publications
11.7K citations
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221 publications · 14.8K citations
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ApJ · 126 publications · 9.7K citations
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37 publications · 2.3K citations
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PRD · 16 publications · 802 citations
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JCAP · 17 publications · 646 citations
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