Intergalactic Ultraviolet Background
The Intergalactic Ultraviolet Background is a diffuse electromagnetic radiation field in the ultraviolet wavelength range that permeates the space between galaxies, originating primarily from the integrated emission of quasars and star-forming galaxies throughout cosmic history.
102
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7.3K
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314
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206
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2017–2026
21
Variants
Intergalactic Uv Background
102
Formation of the First Supermassive Black Holes
Volker Bromm, Abraham Loeb · The Astrophysical Journal · 2003 · 805 citations · Full text
Natural Sciences, Astronomy, Physics +14
R. J. Bouwens, G. D. Illingworth, John P. Blakeslee et al. · The Astrophysical Journal · 2006 · 354 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Max Planck Institute for Astronomy
Heidelberg, Germany
12 h-index
18 publications
1.4K citations

Johns Hopkins University
Baltimore, United States
8 h-index
10 publications
574 citations
University of California, Santa Cruz
Santa Cruz, United States
8 h-index
11 publications
2.2K citations
Leiden University
Leiden, The Netherlands
8 h-index
12 publications
992 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
7 h-index
13 publications
855 citations

Space Telescope Science Institute
Baltimore, United States
7 h-index
26 publications
3.5K citations
University of Cambridge
Cambridge, United Kingdom
7 h-index
14 publications
2.2K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
5 h-index
9 publications
380 citations
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ApJ · 39 publications · 3.7K citations
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25 publications · 1.8K citations
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8 publications · 382 citations
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Repository · 4 publications · 267 citations
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