Globular Cluster Luminosity Function

Globular Cluster Luminosity Function is a statistical model that describes the distribution of luminosities of globular clusters in a galaxy, serving as a standard candle method for estimating extragalactic distances based on the characteristic peak in their brightness distribution.

581

Publications

38K

Citations

1K

Authors

388

Institutions

Publications per year

2017–2026

46

Variants

Gclf

Authors

1K

  1. WE
    William E. Harris

    McMaster University, Canada

    41 publications · 6.8K citations

    24

    h-index

  2. JP
    John P. Blakeslee

    Johns Hopkins University, United States

    17 publications · 1.4K citations

    17

    h-index

  3. PB
    P. B. Stetson

    Herzberg Institute of Astrophysics, Canada

    16 publications · 2K citations

    16

    h-index

  4. HB
    Harvey B. Richer

    University of British Columbia, Canada

    15 publications · 1.1K citations

    14

    h-index

  5. GG
    Gregory G. Fahlman

    University of British Columbia, Canada

    14 publications · 676 citations

    14

    h-index

1–5 of 1K

Venues

  1. The Astrophysical Journal

    ApJ · 190 publications · 11.4K citations

    58

    h-index

  2. The Astronomical Journal

    AJ · 129 publications · 12.8K citations

    51

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    86 publications · 4.9K citations

    42

    h-index

  4. Astronomy and Astrophysics

    40 publications · 2.1K citations

    25

    h-index

  5. The Astrophysical Journal Supplement Series

    14 publications · 1.1K citations

    13

    h-index

1–5