Silicate Feature Analysis is a spectroscopic method in mid-infrared astronomy that identifies and quantifies the characteristic emission or absorption features of silicate minerals in astronomical spectra to infer the physical and chemical properties of interstellar dust.
127
Publications
7.9K
Citations
417
Authors
205
Institutions
Publications per year
2017–2026
10
Parents
Publications
127
1–5 of 127
Authors
417
- MS
6
h-index
- ME
5
h-index
- CM
5
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- CK
4
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- SK
4
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1–5 of 417
Institutions
205
California Institute of Technology
Pasadena, United States
14 h-index
26 publications
2.7K citations
Ames Research Center
Mountain View, United States
11 h-index
25 publications
2K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
19 publications
1.2K citations
University of Kentucky
Lexington, United States
8 h-index
10 publications
1.5K citations
Jet Propulsion Laboratory
Pasadena, United States
8 h-index
14 publications
1K citations
University of Florida
Gainesville, United States
7 h-index
15 publications
839 citations
Centre National de la Recherche Scientifique
Paris, France
7 h-index
13 publications
503 citations
Planetary Science Institute
Tucson, United States
7 h-index
10 publications
536 citations
1–8 of 205
Venues
- The Astrophysical Journal
ApJ · 49 publications · 4.1K citations
33
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- The Astronomical Journal
AJ · 11 publications · 359 citations
11
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- Astronomy and Astrophysics
10 publications · 600 citations
10
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- Icarus
7 publications · 368 citations
7
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- Monthly Notices of the Royal Astronomical Society
6 publications · 147 citations
6
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1–5