X-ray Background Source Counts

X-Ray Background Source Counts is a metric that quantifies the number of discrete astrophysical sources contributing to the diffuse X-ray background radiation per unit area of the sky and per unit flux or sensitivity interval.

105

Publications

7.7K

Citations

455

Authors

193

Institutions

Publications per year

2017–2026

10

Variants

X-ray Background Log N-log S

Authors

455

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    8 publications · 273 citations

    8

    h-index

  2. RG
    R. Gilli

    University of Bologna, Italy

    7 publications · 1.8K citations

    7

    h-index

  3. TM
    T. Maccacaro

    Brera Astronomical Observatory, Italy

    5 publications · 263 citations

    5

    h-index

  4. AC
    A. Comastri

    Osservatorio astronomico di Bologna, Italy

    5 publications · 1.3K citations

    5

    h-index

  5. GP
    G. P. Garmire

    Pennsylvania State University, United States

    5 publications · 751 citations

    5

    h-index

1–5 of 455

Venues

  1. The Astrophysical Journal

    ApJ · 33 publications · 2.3K citations

    24

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.1K citations

    18

    h-index

  3. Astronomy and Astrophysics

    8 publications · 1.4K citations

    8

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 742 citations

    3

    h-index

  5. Advances in Space Research

    2 publications · 45 citations

    2

    h-index

1–5