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
83
Cosmological Simulations with TreeSPH
Neal Katz, David H. Weinberg, Lars Hernquist · The Astrophysical Journal Supplement Series · 1996 · 970 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 83
249
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Kavli Institute for Particle Astrophysics and Cosmology, United States
5 publications · 768 citations
5
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5
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5
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1–5 of 249
163
University of California, Santa Cruz
Santa Cruz, United States
10 h-index
13 publications
2.2K citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
32 publications
1.4K citations
University of Cambridge
Cambridge, United Kingdom
8 h-index
19 publications
2.3K citations
University of California San Diego
San Diego, United States
6 h-index
25 publications
1.3K citations
University of Oxford
Oxford, United Kingdom
6 h-index
9 publications
617 citations
Max Planck Institute for Astrophysics
Garching, Germany
6 h-index
7 publications
1.3K citations
The Ohio State University
Columbus, United States
6 h-index
10 publications
833 citations
Leiden University
Leiden, The Netherlands
5 h-index
12 publications
1.2K citations
1–8 of 163
44 publications · 3.6K citations
28
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ApJ · 19 publications · 2.2K citations
18
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Repository · 3 publications · 157 citations
3
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3 publications · 166 citations
3
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4 publications · 101 citations
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