Initial Mass Function Reconstruction

Initial Mass Function Reconstruction is a computational method in astrophysics that belongs to the class of stellar population modeling techniques, specifically distinguished by its aim to infer the distribution of stellar masses at birth from observed photometric or spectroscopic data of stellar populations.

95

Publications

6K

Citations

374

Authors

206

Institutions

Publications per year

2017–2026

23

Authors

374

  1. MG
    M. G. Petr-Gotzens

    European Southern Observatory, Germany

    5 publications · 130 citations

    5

    h-index

  2. HB
    H. Bouy

    Centro de Astrobiología, Spain

    4 publications · 147 citations

    4

    h-index

  3. NH
    N. Huélamo

    Centro de Astrobiología, Spain

    4 publications · 91 citations

    4

    h-index

  4. AB
    A. Bayo

    University of Valparaíso, Chile

    3 publications · 68 citations

    3

    h-index

  5. EM
    Enrico Marchetti

    European Southern Observatory, Germany

    3 publications · 72 citations

    3

    h-index

1–5 of 374

Venues

  1. The Astrophysical Journal

    ApJ · 26 publications · 1.9K citations

    23

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.6K citations

    20

    h-index

  3. Astronomy and Astrophysics

    11 publications · 707 citations

    11

    h-index

  4. The Astronomical Journal

    AJ · 6 publications · 395 citations

    6

    h-index

  5. Journal of High Energy Physics

    JHEP · 3 publications · 83 citations

    3

    h-index

1–5