Galactic Dust Attenuation
Galactic Dust Attenuation is a physical process in astrophysics whereby interstellar dust grains within the Milky Way preferentially absorb and scatter shorter-wavelength electromagnetic radiation, thereby diminishing the observed flux and reddening the spectral energy distribution of background astronomical sources.
177
Publications
16.2K
Citations
893
Authors
342
Institutions
Publications per year
2017–2026
83
Parents
177
UV Star Formation Rates in the Local Universe
The Astrophysical Journal Supplement Series · 2007 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
Vicente Rodríguez-Gómez, Gregory F. Snyder, Jennifer M. Lotz et al. · Monthly Notices of the Royal Astronomical Society · 2018 · 445 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 177
893
10
h-index
Center for Astrophysics Harvard & Smithsonian, United States
9 publications · 1.2K citations
9
h-index
8
h-index
8
h-index
7
h-index
1–5 of 893
342

Centre National de la Recherche Scientifique
Paris, France
31 h-index
79 publications
7.6K citations
California Institute of Technology
Pasadena, United States
27 h-index
92 publications
19.5K citations

Space Telescope Science Institute
Baltimore, United States
22 h-index
64 publications
5.2K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
18 h-index
43 publications
3.2K citations
Laboratoire d’Astrophysique de Marseille
Marseille, France
17 h-index
44 publications
8K citations

University of Massachusetts Amherst
Amherst Center, United States
16 h-index
26 publications
2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
38 publications
6.2K citations
University of Arizona
Tucson, United States
16 h-index
48 publications
3.1K citations
1–8 of 342
ApJ · 56 publications · 6.8K citations
39
h-index
59 publications · 4.2K citations
38
h-index
14 publications · 906 citations
13
h-index
6 publications · 1.9K citations
6
h-index
5 publications · 581 citations
5
h-index
1–5