Ultraviolet Background Emissivity
Ultraviolet Background Emissivity is a radiative property that quantifies the intrinsic emission rate of ultraviolet photons per unit volume, wavelength, and time from diffuse sources in the intergalactic medium, distinguishing it from related radiative transfer quantities by characterizing the specific contribution of pervasive, non-local sources to the cosmic ultraviolet background radiation field.
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2K
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118
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74
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2017–2026
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Color-selected galaxies at z~6 in the Great Observatories Origins Deep Survey
2003 · 185 citations · Full text
Natural Sciences, Astronomy, Physics +13
Ewald Puchwein, Francesco Haardt, Martin G. Haehnelt et al. · Monthly Notices of the Royal Astronomical Society · 2019 · 176 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Centre National de la Recherche Scientifique
Paris, France
3 h-index
5 publications
342 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
4 publications
701 citations

University of Edinburgh
Edinburgh, United Kingdom
3 h-index
4 publications
355 citations
Leiden University
Leiden, The Netherlands
3 h-index
12 publications
1.1K citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
2 h-index
3 publications
308 citations
Institute of Astronomy
Moscow, Russia
2 h-index
5 publications
106 citations
Royal Observatory
Edinburgh, United Kingdom
2 h-index
5 publications
301 citations

UK Astronomy Technology Centre
Edinburgh, United Kingdom
2 h-index
2 publications
99 citations
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10 publications · 986 citations
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ApJ · 5 publications · 152 citations
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3 publications · 211 citations
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2 publications · 52 citations
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1 publications · 24 citations
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