X-ray Background Intensity

X-Ray Background Intensity is a radiometric quantity that denotes the flux density of diffuse X-ray photons per unit energy, area, solid angle, and time, originating from unresolved cosmic sources and instrumental background, thereby characterizing the overall brightness of the X-ray background radiation field.

318

Publications

17.3K

Citations

1.1K

Authors

337

Institutions

Publications per year

2017–2026

14

Authors

1.1K

  1. DM
    D. McCammon

    University of Wisconsin–Madison, United States

    8 publications · 1K citations

    8

    h-index

  2. TD
    Tadayasu Dotani

    Institute of Space and Astronautical Science, Japan

    7 publications · 135 citations

    7

    h-index

  3. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    6 publications · 125 citations

    6

    h-index

  4. EA
    E. A. Boldt

    Goddard Space Flight Center, United States

    6 publications · 405 citations

    6

    h-index

  5. NY
    Noriko Y. Yamasaki

    Institute of Space and Astronautical Science, Japan

    5 publications · 592 citations

    5

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 91 publications · 5.9K citations

    38

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    29 publications · 1.3K citations

    23

    h-index

  3. Nature

    10 publications · 774 citations

    10

    h-index

  4. Review of Scientific Instruments

    8 publications · 369 citations

    8

    h-index

  5. X-Ray Spectrometry

    7 publications · 188 citations

    7

    h-index

1–5