Intergalactic Medium Contribution

Intergalactic Medium Contribution is a theoretical construct in astrophysics that denotes the specific component of the X-ray background radiation arising from diffuse, hot plasma located in the intergalactic space, distinguished from other sources by its spatial distribution and thermal emission characteristics.

1.4K

Publications

110.2K

Citations

4.1K

Authors

877

Institutions

Publications per year

2017–2026

385

Authors

4.1K

  1. MG
    Martin G. Haehnelt

    University of Cambridge, United Kingdom

    41 publications · 4K citations

    30

    h-index

  2. AM
    Andrei Mesinger

    Scuola Normale Superiore, Italy

    40 publications · 4K citations

    29

    h-index

  3. SR
    Steven R. Furlanetto

    University of California, Los Angeles, United States

    32 publications · 3.8K citations

    27

    h-index

  4. AF
    Andrea Ferrara

    Scuola Normale Superiore, Italy

    30 publications · 2.5K citations

    26

    h-index

  5. JX
    J. X. Prochaska

    University of California, Santa Cruz, United States

    31 publications · 3.7K citations

    25

    h-index

1–5 of 4.1K

Venues

  1. The Astrophysical Journal

    ApJ · 504 publications · 45.6K citations

    114

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    423 publications · 30.4K citations

    94

    h-index

  3. Astronomy and Astrophysics

    54 publications · 2.8K citations

    33

    h-index

  4. The Astrophysical Journal Letters

    35 publications · 3.7K citations

    30

    h-index

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

    Repository · 30 publications · 2.2K citations

    26

    h-index

1–5