X-ray Background Cross-correlation

X-Ray Background Cross-Correlation is a statistical method used in astrophysics that quantifies the spatial or angular correlation between X-ray background intensity fluctuations and other cosmological observables to disentangle their shared large-scale structure origins and underlying source populations.

21

Publications

761

Citations

100

Authors

75

Institutions

Publications per year

2017–2026

5

Authors

100

  1. AF
    A. Finoguenov

    Max Planck Institute for Extraterrestrial Physics, Germany

    3 publications · 184 citations

    3

    h-index

  2. SP
    S. P. Boughn

    Haverford College, United States

    2 publications · 48 citations

    2

    h-index

  3. NC
    N. Cappelluti

    Max Planck Institute for Extraterrestrial Physics, Germany

    2 publications · 137 citations

    2

    h-index

  4. RG
    Richard G. Arendt

    Goddard Space Flight Center, United States

    2 publications · 137 citations

    2

    h-index

  5. GH
    G. Hasinger

    Max Planck Institute for Extraterrestrial Physics, Germany

    2 publications · 137 citations

    2

    h-index

1–5 of 100

Venues

  1. 7

    h-index

  2. The Astrophysical Journal

    ApJ · 6 publications · 250 citations

    6

    h-index

  3. The Astronomical Journal

    AJ · 2 publications · 52 citations

    2

    h-index

  4. Astronomy and Astrophysics

    1 publications · 14 citations

    1

    h-index

  5. Nature Photonics

    1 publications · 148 citations

    1

    h-index

1–5