Soft X-ray Background

The Soft X-Ray Background is a diffuse cosmic radiation component within the X-Ray Background Radiation spectrum, distinguished by its photon energies in the 0.1–2 keV range, primarily originating from hot interstellar plasma and unresolved astrophysical sources.

1.5K

Publications

84.3K

Citations

3.5K

Authors

864

Institutions

Publications per year

2017–2026

148

Authors

3.5K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    49 publications · 3.5K citations

    32

    h-index

  2. CD
    Chris Done

    Durham University, United Kingdom

    26 publications · 2.5K citations

    23

    h-index

  3. GM
    G. Matt

    Roma Tre University, Italy

    24 publications · 1K citations

    20

    h-index

  4. DM
    D. McCammon

    University of Wisconsin–Madison, United States

    26 publications · 2.6K citations

    19

    h-index

  5. WT
    W. T. Sanders

    University of Wisconsin–Madison, United States

    21 publications · 2.6K citations

    18

    h-index

1–5 of 3.5K

Venues

  1. The Astrophysical Journal

    ApJ · 526 publications · 38.2K citations

    95

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    281 publications · 16K citations

    65

    h-index

  3. Astronomy and Astrophysics

    147 publications · 8.1K citations

    47

    h-index

  4. Publications of the Astronomical Society of Japan

    38 publications · 1.6K citations

    23

    h-index

  5. Solar Physics

    31 publications · 1.2K citations

    18

    h-index

1–5