Simple Stellar Populations
Simple Stellar Populations is a theoretical astrophysical model representing a coeval, chemically homogeneous group of stars formed at the same time and location, distinguished by its assumption of negligible spread in age and metallicity, used to study the collective evolution of stars within a single stellar generation.
374
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29.8K
Citations
1.1K
Authors
436
Institutions
Publications per year
2017–2026
65
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Ssps
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374
CIGALE: a python Code Investigating GALaxy Emission
M. Boquien, D. Burgarella, Y. Roehlly et al. · Astronomy and Astrophysics · 2018 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +17
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Space Telescope Science Institute
Baltimore, United States
28 h-index
71 publications
4.3K citations
European Southern Observatory
Garching bei München, Germany
25 h-index
56 publications
7.9K citations
Osservatorio Astronomico di Padova
Padua, Italy
23 h-index
99 publications
7K citations
University of California, Santa Cruz
Santa Cruz, United States
23 h-index
41 publications
4.9K citations

Centre National de la Recherche Scientifique
Paris, France
21 h-index
42 publications
10.6K citations
Liverpool John Moores University
Liverpool, United Kingdom
21 h-index
53 publications
2.4K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
20 h-index
34 publications
5.4K citations
National Astronomical Observatories
Beijing, China
18 h-index
75 publications
4K citations
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104 publications · 8K citations
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ApJ · 75 publications · 7.2K citations
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54 publications · 4.3K citations
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AJ · 31 publications · 2.1K citations
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13 publications · 978 citations
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