Initial Mass Function Normalization

Initial Mass Function Normalization is a methodological framework in astrophysics that standardizes the initial mass function by scaling its integral over stellar masses to unity, thereby enabling consistent comparison of star formation rates and population synthesis models across different galactic environments.

225

Publications

28.2K

Citations

730

Authors

334

Institutions

Publications per year

2017–2026

47

Authors

730

  1. LV
    L. V. E. Koopmans

    University of Groningen, Netherlands

    7 publications · 664 citations

    7

    h-index

  2. MC
    Michele Cappellari

    University of Oxford, United Kingdom

    7 publications · 1.6K citations

    7

    h-index

  3. RL
    Roger L. Davies

    University of Oxford, United Kingdom

    6 publications · 1.5K citations

    6

    h-index

  4. TT
    Tommaso Treu

    University of California, Los Angeles, United States

    5 publications · 386 citations

    5

    h-index

  5. CT
    C. Tortora

    Astronomical Observatory of Capodimonte, Italy

    5 publications · 198 citations

    5

    h-index

1–5 of 730

Venues

  1. The Astrophysical Journal

    ApJ · 67 publications · 7.2K citations

    44

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    63 publications · 13.7K citations

    36

    h-index

  3. Astronomy and Astrophysics

    17 publications · 569 citations

    15

    h-index

  4. The Astronomical Journal

    AJ · 16 publications · 1.6K citations

    14

    h-index

  5. The Astrophysical Journal Letters

    8 publications · 564 citations

    8

    h-index

1–5