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
100
The Radiative Feedback of the First Cosmological Objects
Zoltán Haiman, Tom Abel, M. J. Rees · The Astrophysical Journal · 2000 · 381 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 100
271
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Inter-University Centre for Astronomy and Astrophysics, India
5 publications · 299 citations
5
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4
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1–5 of 271
180
University of California, Santa Cruz
Santa Cruz, United States
9 h-index
13 publications
3.8K citations
University of Cambridge
Cambridge, United Kingdom
9 h-index
21 publications
2K citations
California Institute of Technology
Pasadena, United States
6 h-index
10 publications
390 citations
University of Insubria
Varese, Italy
6 h-index
6 publications
1.8K citations
The Ohio State University
Columbus, United States
5 h-index
8 publications
569 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
5 h-index
8 publications
682 citations
Inter-University Centre for Astronomy and Astrophysics
Pune, India
5 h-index
9 publications
444 citations

Johns Hopkins University
Baltimore, United States
5 h-index
5 publications
220 citations
1–8 of 180
42 publications · 2.9K citations
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ApJ · 25 publications · 5.5K citations
21
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3 publications · 190 citations
3
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1 publications · 82 citations
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Repository · 2 publications · 94 citations
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