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.

580

Publications

37.8K

Citations

2.1K

Authors

556

Institutions

Publications per year

2017–2026

207

Authors

2.1K

  1. RM
    Rachel Mandelbaum

    Carnegie Mellon University, United States

    30 publications · 4.3K citations

    29

    h-index

  2. EG
    E. Gaztañaga

    Institute of Space Sciences, Spain

    23 publications · 1.4K citations

    18

    h-index

  3. EK
    E. Krause

    The Ohio State University, United States

    19 publications · 1.3K citations

    18

    h-index

  4. HH
    H. Hildebrandt

    Leiden University, Netherlands

    21 publications · 1.9K citations

    18

    h-index

  5. CH
    Catherine Heymans

    University of Edinburgh, United Kingdom

    21 publications · 1.9K citations

    18

    h-index

1–5 of 2.1K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    221 publications · 14.8K citations

    66

    h-index

  2. The Astrophysical Journal

    ApJ · 126 publications · 9.7K citations

    55

    h-index

  3. Astronomy and Astrophysics

    37 publications · 2.3K citations

    25

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 16 publications · 802 citations

    16

    h-index

  5. Journal of Cosmology and Astroparticle Physics

    JCAP · 17 publications · 646 citations

    14

    h-index

1–5