Stellar Luminosities

Stellar Luminosities is a photometric metric that quantifies the total radiant energy emitted by a star per unit time, differentiating it from apparent brightness by representing intrinsic stellar emission rather than observed flux attenuated by distance and extinction.

1.3K

Publications

101.2K

Citations

4.1K

Authors

880

Institutions

Publications per year

2017–2026

211

Authors

4.1K

  1. OJ
    O. J. Eggen

    Cerro Tololo Inter-American Observatory, Chile

    18 publications · 360 citations

    13

    h-index

  2. MM
    M. Mignoli

    Osservatorio astronomico di Bologna, Italy

    11 publications · 2.3K citations

    11

    h-index

  3. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    10 publications · 708 citations

    10

    h-index

  4. TS
    T. Shenar

    University of Potsdam, Germany

    10 publications · 773 citations

    10

    h-index

  5. CV
    C. Vignali

    University of Bologna, Italy

    10 publications · 741 citations

    10

    h-index

1–5 of 4.1K

Venues

  1. The Astrophysical Journal

    ApJ · 497 publications · 41.8K citations

    102

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    222 publications · 14.9K citations

    68

    h-index

  3. Astronomy and Astrophysics

    133 publications · 8.7K citations

    54

    h-index

  4. The Astronomical Journal

    AJ · 110 publications · 12.2K citations

    53

    h-index

  5. The Astrophysical Journal Supplement Series

    41 publications · 6.2K citations

    33

    h-index

1–5