Stellar Population Synthesis

Stellar Population Synthesis is a theoretical framework in astrophysics that models the collective spectral energy distribution of a stellar population by combining the evolutionary tracks, spectral properties, and relative abundances of individual stars to infer intrinsic galactic properties such as age, metallicity, and star formation history.

858

Publications

101.7K

Citations

2.1K

Authors

635

Institutions

Publications per year

2017–2026

190

Authors

2.1K

  1. CJ
    C. J. Evans

    UK Astronomy Technology Centre, United Kingdom

    33 publications · 3.2K citations

    29

    h-index

  2. HS
    H. Sana

    KU Leuven, Belgium

    31 publications · 3.1K citations

    28

    h-index

  3. JS
    J. S. Vink

    Armagh Observatory & Planetarium, United Kingdom

    26 publications · 2.7K citations

    24

    h-index

  4. AD
    A. de Koter

    University of Amsterdam, Netherlands

    24 publications · 2.7K citations

    23

    h-index

  5. WD
    W. D. Taylor

    UK Astronomy Technology Centre, United Kingdom

    26 publications · 2.8K citations

    23

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 210 publications · 25.5K citations

    75

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    230 publications · 33.9K citations

    71

    h-index

  3. Astronomy and Astrophysics

    142 publications · 11K citations

    61

    h-index

  4. The Astrophysical Journal Supplement Series

    35 publications · 8.9K citations

    27

    h-index

  5. The Astronomical Journal

    AJ · 35 publications · 3.7K citations

    25

    h-index

1–5