Interstellar Dust Attenuation
Interstellar Dust Attenuation is a radiative transfer phenomenon in which ultraviolet light from extragalactic sources is selectively absorbed and scattered by interstellar dust grains, thereby reducing observed flux and altering spectral energy distributions in a wavelength-dependent manner.
158
Publications
14.6K
Citations
860
Authors
357
Institutions
Publications per year
2017–2026
77
158
A Simple Model for the Absorption of Starlight by Dust in Galaxies
S. Charlot, S. Michael Fall · The Astrophysical Journal · 2000 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +15
UV Star Formation Rates in the Local Universe
The Astrophysical Journal Supplement Series · 2007 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
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357

Centre National de la Recherche Scientifique
Paris, France
27 h-index
81 publications
7.9K citations

Space Telescope Science Institute
Baltimore, United States
22 h-index
63 publications
6.6K citations
University of Arizona
Tucson, United States
19 h-index
55 publications
4K citations
Institut d'Astrophysique de Paris
Paris, France
16 h-index
20 publications
5.4K citations
Laboratoire d’Astrophysique de Marseille
Marseille, France
16 h-index
42 publications
6.2K citations

University of Massachusetts Amherst
Amherst Center, United States
15 h-index
27 publications
2.6K citations
California Institute of Technology
Pasadena, United States
14 h-index
40 publications
13.7K citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
13 h-index
23 publications
874 citations
1–8 of 357
ApJ · 52 publications · 6.3K citations
35
h-index
46 publications · 3.4K citations
33
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19 publications · 914 citations
18
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8 publications · 678 citations
7
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AJ · 5 publications · 347 citations
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