Source Number Counts

Source Number Counts is a statistical metric in X-ray astronomy that characterizes the cumulative number of detected X-ray sources per unit area as a function of flux, distinguishing itself by quantifying the source density distribution to probe cosmological populations and instrument sensitivity.

711

Publications

55.5K

Citations

3.7K

Authors

744

Institutions

Publications per year

2017–2026

114

Variants

Log N - Log S

Authors

3.7K

  1. RJ
    R. J. Ivison

    Royal Observatory, United Kingdom

    28 publications · 4.8K citations

    25

    h-index

  2. DS
    D. Scott

    University of British Columbia, Canada

    25 publications · 3.9K citations

    24

    h-index

  3. GZ
    G. Zamorani

    University of Bologna, Italy

    24 publications · 1.9K citations

    19

    h-index

  4. SS
    S. Serjeant

    The Open University, United Kingdom

    19 publications · 2.2K citations

    17

    h-index

  5. DL
    D. L. Clements

    Imperial College London, United Kingdom

    17 publications · 3K citations

    16

    h-index

1–5 of 3.7K

Venues

  1. The Astrophysical Journal

    ApJ · 165 publications · 12.7K citations

    64

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    206 publications · 13.9K citations

    62

    h-index

  3. Astronomy and Astrophysics

    81 publications · 7.7K citations

    39

    h-index

  4. The Astrophysical Journal Supplement Series

    37 publications · 6.6K citations

    28

    h-index

  5. The Astronomical Journal

    AJ · 25 publications · 2.8K citations

    19

    h-index

1–5