Stellar Population Synthesis
Stellar Population Synthesis is a theoretical framework in astrophysics that models the collective spectral energy distribution of a stellar population by combining the evolutionary tracks, spectral properties, and relative abundances of individual stars to infer intrinsic galactic properties such as age, metallicity, and star formation history.
858
Publications
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Citations
2.1K
Authors
635
Institutions
Publications per year
2017–2026
190
Variants
Population Synthesis
858
Charlie Conroy, James E. Gunn, Martin White · The Astrophysical Journal · 2009 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
47 h-index
191 publications
39.1K citations

Space Telescope Science Institute
Baltimore, United States
46 h-index
133 publications
38.9K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
43 h-index
112 publications
20.2K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
35 h-index
91 publications
12.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
35 h-index
90 publications
9.1K citations
Royal Observatory
Edinburgh, United Kingdom
33 h-index
99 publications
17.1K citations
European Southern Observatory
Garching bei München, Germany
32 h-index
58 publications
8.4K citations
Instituto de Astrofísica de Andalucía
Granada, Spain
32 h-index
63 publications
12.3K citations
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ApJ · 210 publications · 25.5K citations
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230 publications · 33.9K citations
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142 publications · 11K citations
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35 publications · 8.9K citations
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AJ · 35 publications · 3.7K citations
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