White Dwarf Luminosity Function

The White Dwarf Luminosity Function is a statistical representation that quantifies the number density of white dwarf stars per unit luminosity interval, serving as a fundamental diagnostic tool in stellar population studies to constrain the age, formation history, and evolution of galactic stellar populations.

172

Publications

11.1K

Citations

297

Authors

167

Institutions

Publications per year

2017–2026

14

Authors

297

  1. JI
    J. Isern

    Institut d'Estudis Espacials de Catalunya, Spain

    22 publications · 1.5K citations

    18

    h-index

  2. EG
    E. Garcı́a–Berro

    Universitat Politècnica de Catalunya, Spain

    20 publications · 924 citations

    16

    h-index

  3. ST
    Santiago Torres

    Universitat Politècnica de Catalunya, Spain

    18 publications · 748 citations

    15

    h-index

  4. JL
    James Liebert

    University of Arizona, United States

    12 publications · 1.9K citations

    12

    h-index

  5. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    9 publications · 511 citations

    9

    h-index

1–5 of 297

Venues

  1. The Astrophysical Journal

    ApJ · 64 publications · 5.7K citations

    45

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    28 publications · 1.7K citations

    23

    h-index

  3. Astronomy and Astrophysics

    14 publications · 445 citations

    13

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 490 citations

    9

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 5 publications · 69 citations

    5

    h-index

1–5