Ultraviolet Background Modeling

Ultraviolet Background Modeling is a computational framework that characterizes the diffuse ultraviolet radiation field in the intergalactic medium by synthesizing contributions from known astrophysical sources and intervening absorption, distinguished from other radiative transfer models by its specificity to the ultraviolet spectrum and large-scale cosmological structure.

100

Publications

10.8K

Citations

271

Authors

180

Institutions

Publications per year

2017–2026

26

Authors

271

  1. MG
    Martin G. Haehnelt

    University of Cambridge, United Kingdom

    6 publications · 528 citations

    6

    h-index

  2. PM
    Piero Madau

    University of California, Santa Cruz, United States

    6 publications · 2.2K citations

    6

    h-index

  3. FH
    Francesco Haardt

    University of Insubria, Italy

    6 publications · 2.2K citations

    6

    h-index

  4. RS
    R. Srianand

    Inter-University Centre for Astronomy and Astrophysics, India

    5 publications · 299 citations

    5

    h-index

  5. EP
    Ewald Puchwein

    University of Cambridge, United Kingdom

    4 publications · 442 citations

    4

    h-index

1–5 of 271

Venues

  1. Monthly Notices of the Royal Astronomical Society

    42 publications · 2.9K citations

    25

    h-index

  2. The Astrophysical Journal

    ApJ · 25 publications · 5.5K citations

    21

    h-index

  3. Astronomy and Astrophysics

    3 publications · 190 citations

    3

    h-index

  4. 2

    h-index

  5. eScholarship (California Digital Library)

    Repository · 2 publications · 94 citations

    2

    h-index

1–5