Stellar Mass Distribution

Stellar Mass Distribution is a theoretical construct in astrophysics that specifies the relative number of stars at each stellar mass within a given population, distinguished from other distribution models by its focus on the statistical arrangement of stellar masses at birth.

2.8K

Publications

258.8K

Citations

7.5K

Authors

1.2K

Institutions

Publications per year

2017–2026

1K

Authors

7.5K

  1. AM
    Anton M. Koekemoer

    Space Telescope Science Institute, United States

    67 publications · 8.8K citations

    48

    h-index

  2. CJ
    Christopher J. Conselice

    University of Nottingham, United Kingdom

    47 publications · 7.7K citations

    37

    h-index

  3. PV
    Pieter van Dokkum

    Yale University, United States

    47 publications · 8.1K citations

    36

    h-index

  4. OI
    O. Ilbert

    Centre National de la Recherche Scientifique, France

    47 publications · 5.5K citations

    35

    h-index

  5. HJ
    H. J. McCracken

    Institut d'Astrophysique de Paris, France

    43 publications · 7.3K citations

    35

    h-index

1–5 of 7.5K

Venues

  1. The Astrophysical Journal

    ApJ · 922 publications · 106.5K citations

    161

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    931 publications · 76K citations

    126

    h-index

  3. Astronomy and Astrophysics

    266 publications · 20.6K citations

    73

    h-index

  4. The Astrophysical Journal Letters

    124 publications · 9.8K citations

    59

    h-index

  5. The Astronomical Journal

    AJ · 82 publications · 6.3K citations

    40

    h-index

1–5