Open Cluster Luminosity Function

Open Cluster Luminosity Function is a statistical construct that characterizes the distribution of absolute magnitudes among open star clusters in a given region of the sky, serving to quantify the number of clusters per unit luminosity interval as a function of brightness.

98

Publications

4.9K

Citations

199

Authors

132

Institutions

Publications per year

2017–2026

9

Authors

199

  1. GC
    G. Carraro

    Osservatorio Astronomico di Padova, Italy

    6 publications · 115 citations

    6

    h-index

  2. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    6 publications · 260 citations

    6

    h-index

  3. RS
    R. Sagar

    Aryabhatta Research Institute of Observational Sciences, India

    5 publications · 159 citations

    5

    h-index

  4. NC
    N. C. Hambly

    University of Edinburgh, United Kingdom

    4 publications · 139 citations

    4

    h-index

  5. ES
    E. Schilbach

    Heidelberg University, Germany

    4 publications · 103 citations

    4

    h-index

1–5 of 199

Venues

  1. Astronomy and Astrophysics

    20 publications · 882 citations

    18

    h-index

  2. The Astronomical Journal

    AJ · 18 publications · 1.3K citations

    17

    h-index

  3. The Astrophysical Journal

    ApJ · 15 publications · 1.2K citations

    14

    h-index

  4. 14

    h-index

  5. New Astronomy

    3 publications · 46 citations

    3

    h-index

1–5