X-ray Background Spectrum

X-Ray Background Spectrum is an observational astrophysical dataset representing the diffuse X-ray emission across the sky, distinguished by its characterization of the intensity and energy distribution of extragalactic and galactic X-ray photons after the removal of discrete sources.

1.5K

Publications

84K

Citations

4.8K

Authors

870

Institutions

Publications per year

2017–2026

189

Authors

4.8K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    71 publications · 4K citations

    36

    h-index

  2. WN
    W. N. Brandt

    Pennsylvania State University, United States

    34 publications · 3.1K citations

    27

    h-index

  3. FE
    F. E. Bauer

    Pontificia Universidad Católica de Chile, Chile

    24 publications · 2.2K citations

    22

    h-index

  4. AC
    A. Comastri

    Osservatorio astronomico di Bologna, Italy

    27 publications · 2.6K citations

    22

    h-index

  5. GM
    G. Matt

    Roma Tre University, Italy

    29 publications · 1.7K citations

    21

    h-index

1–5 of 4.8K

Venues

  1. The Astrophysical Journal

    ApJ · 529 publications · 34.1K citations

    88

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    273 publications · 15K citations

    63

    h-index

  3. Astronomy and Astrophysics

    140 publications · 8K citations

    49

    h-index

  4. Nature

    42 publications · 2.6K citations

    26

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 34 publications · 1.7K citations

    22

    h-index

1–5