Lens Reconstruction
Lens Reconstruction is a computational method in astrophysics that distinguishes itself by inferring the mass distribution of a gravitational lens from observed distortions in background light sources, within the broader class of techniques used to model gravitational lensing phenomena.
174
Publications
9.3K
Citations
687
Authors
307
Institutions
Publications per year
2017–2026
61
Parents
174
Matthias Bartelmann · Classical and Quantum Gravity · 2010 · 439 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 174
687
12
h-index
8
h-index
8
h-index
8
h-index
7
h-index
1–5 of 687
307
University of Cambridge
Cambridge, United Kingdom
14 h-index
37 publications
2.1K citations
Kavli Institute for Particle Astrophysics and Cosmology
Menlo Park, United States
14 h-index
33 publications
2.9K citations

University of Minnesota
Minneapolis, United States
14 h-index
24 publications
1.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
30 publications
2.3K citations
University of California, Berkeley
Berkeley, United States
12 h-index
29 publications
1.3K citations
University of Chicago
Chicago, United States
12 h-index
65 publications
3.9K citations
California Institute of Technology
Pasadena, United States
12 h-index
33 publications
2.7K citations
Max Planck Institute for Astrophysics
Garching, Germany
12 h-index
21 publications
1.1K citations
1–8 of 307
ApJ · 33 publications · 2K citations
28
h-index
51 publications · 2.6K citations
27
h-index
13 publications · 422 citations
13
h-index
PRD · 12 publications · 453 citations
12
h-index
JCAP · 8 publications · 483 citations
8
h-index
1–5