Bulge-disk Decomposition

Bulge-Disk Decomposition is a quantitative image analysis method in galaxy morphology that separates a galaxy’s light distribution into structurally distinct components—specifically a centrally concentrated bulge and an extended disk—by fitting two-dimensional surface brightness profiles to distinguish their photometric and structural properties.

284

Publications

22.8K

Citations

851

Authors

370

Institutions

Publications per year

2017–2026

66

Variants

Bulge-to-disk DecompositionBulge/disk Decomposition

Authors

851

  1. AW
    Alister W. Graham

    Swinburne University of Technology, Australia

    12 publications · 1.5K citations

    12

    h-index

  2. LS
    Luc Simard

    Herzberg Institute of Astrophysics, Canada

    12 publications · 1.9K citations

    12

    h-index

  3. SP
    Simon P. Driver

    The University of Western Australia, Australia

    9 publications · 1K citations

    9

    h-index

  4. DC
    David C. Koo

    University of California, Santa Cruz, United States

    9 publications · 997 citations

    9

    h-index

  5. MB
    M. Balcells

    Instituto de Astrofísica de Canarias, Spain

    8 publications · 596 citations

    8

    h-index

1–5 of 851

Venues

  1. Monthly Notices of the Royal Astronomical Society

    78 publications · 6.3K citations

    44

    h-index

  2. The Astrophysical Journal

    ApJ · 64 publications · 5.5K citations

    43

    h-index

  3. The Astronomical Journal

    AJ · 27 publications · 1.9K citations

    24

    h-index

  4. Astronomy and Astrophysics

    29 publications · 1.5K citations

    21

    h-index

  5. The Astrophysical Journal Supplement Series

    19 publications · 3.3K citations

    18

    h-index

1–5