X-ray Background Modeling

X-Ray Background Modeling is a scientific method that characterizes the diffuse X-ray emission originating from cosmic sources and instrumental backgrounds by distinguishing astrophysical signals from contaminating components through statistical and physical modeling techniques.

291

Publications

19.6K

Citations

774

Authors

322

Institutions

Publications per year

2017–2026

41

Authors

774

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    21 publications · 1.3K citations

    16

    h-index

  2. AC
    A. Comastri

    Osservatorio astronomico di Bologna, Italy

    11 publications · 1.3K citations

    10

    h-index

  3. RG
    R. Gilli

    University of Bologna, Italy

    10 publications · 1.4K citations

    10

    h-index

  4. XB
    X. Barcons

    Instituto de Física de Cantabria, Spain

    8 publications · 291 citations

    8

    h-index

  5. KJ
    K. Jahoda

    Goddard Space Flight Center, United States

    7 publications · 261 citations

    7

    h-index

1–5 of 774

Venues

  1. The Astrophysical Journal

    ApJ · 82 publications · 6.2K citations

    41

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    56 publications · 3.6K citations

    33

    h-index

  3. Astronomy and Astrophysics

    24 publications · 2.3K citations

    18

    h-index

  4. Nature

    7 publications · 185 citations

    7

    h-index

  5. 5

    h-index

1–5