Ultraviolet Background Simulations

Ultraviolet Background Simulations is a computational modeling framework that generates synthetic representations of the diffuse ultraviolet radiation field permeating intergalactic and circumgalactic media, distinguished by its incorporation of cosmological structure formation, radiative transfer physics, and quasar-galaxy emissivity evolution to predict the ionization state of the high-redshift universe.

83

Publications

8.1K

Citations

249

Authors

163

Institutions

Publications per year

2017–2026

23

Authors

249

  1. MG
    Martin G. Haehnelt

    University of Cambridge, United Kingdom

    6 publications · 597 citations

    6

    h-index

  2. ML
    Michael L. Norman

    University of California San Diego, United States

    5 publications · 353 citations

    5

    h-index

  3. TA
    Tom Abel

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    5 publications · 768 citations

    5

    h-index

  4. TT
    Tom Theuns

    Durham University, United Kingdom

    5 publications · 924 citations

    5

    h-index

  5. PM
    Piero Madau

    University of California, Santa Cruz, United States

    5 publications · 594 citations

    5

    h-index

1–5 of 249

Venues

  1. Monthly Notices of the Royal Astronomical Society

    44 publications · 3.6K citations

    28

    h-index

  2. The Astrophysical Journal

    ApJ · 19 publications · 2.2K citations

    18

    h-index

  3. arXiv (Cornell University)

    Repository · 3 publications · 157 citations

    3

    h-index

  4. The Astrophysical Journal Letters

    3 publications · 166 citations

    3

    h-index

  5. Astronomy and Astrophysics

    4 publications · 101 citations

    3

    h-index

1–5