X-ray Luminosity Functions

X-Ray Luminosity Functions is a statistical framework in astrophysics that describes the number density of X-ray-emitting sources per unit luminosity interval, distinguishing itself by quantifying the distribution of X-ray luminosities across populations of extragalactic or Galactic sources to characterize their emission properties and evolution.

2K

Publications

147.4K

Citations

4.5K

Authors

937

Institutions

Publications per year

2017–2026

301

Variants

X-ray Luminosity Function

Authors

4.5K

  1. WN
    W. N. Brandt

    Pennsylvania State University, United States

    44 publications · 3.9K citations

    33

    h-index

  2. MB
    M. Brusa

    University of Bologna, Italy

    38 publications · 4.1K citations

    32

    h-index

  3. AC
    A. Comastri

    Osservatorio astronomico di Bologna, Italy

    41 publications · 4.8K citations

    31

    h-index

  4. CV
    C. Vignali

    University of Bologna, Italy

    38 publications · 3.5K citations

    30

    h-index

  5. MS
    M. Salvato

    Max Planck Institute for Extraterrestrial Physics, Germany

    41 publications · 5.8K citations

    30

    h-index

1–5 of 4.5K

Venues

  1. The Astrophysical Journal

    ApJ · 777 publications · 62.8K citations

    121

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    501 publications · 36.8K citations

    96

    h-index

  3. Astronomy and Astrophysics

    236 publications · 18.8K citations

    66

    h-index

  4. The Astrophysical Journal Supplement Series

    40 publications · 5.2K citations

    34

    h-index

  5. The Astronomical Journal

    AJ · 68 publications · 3.8K citations

    32

    h-index

1–5