Lensing By Compact Objects

Lensing By Compact Objects is a theoretical framework in gravitational lensing that specifically models the bending of light caused by the strong gravitational fields of dense, localized masses such as black holes, neutron stars, or white dwarfs, distinguishing it from lensing by extended or diffuse mass distributions.

196

Publications

13.6K

Citations

1.9K

Authors

324

Institutions

Publications per year

2017–2026

71

Authors

1.9K

  1. AG
    Andrew Gould

    The Ohio State University, United States

    8 publications · 1.1K citations

    8

    h-index

  2. CR
    Charles R. Keeton

    Rutgers, The State University of New Jersey, United States

    6 publications · 573 citations

    6

    h-index

  3. NT
    Naoki Tsukamoto

    National Institute of Technology, Japan

    5 publications · 511 citations

    5

    h-index

  4. AO
    A. O. Petters

    Duke University, United States

    5 publications · 464 citations

    5

    h-index

  5. DS
    Dominique Sluse

    École Polytechnique Fédérale de Lausanne, Switzerland

    4 publications · 213 citations

    4

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 56 publications · 4.5K citations

    30

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    35 publications · 1.7K citations

    24

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 17 publications · 1.4K citations

    16

    h-index

  4. Astronomy and Astrophysics

    12 publications · 634 citations

    12

    h-index

  5. 10

    h-index

1–5