Galaxy Color Evolution
Galaxy Color Evolution is a theoretical construct in astrophysics that characterizes the systematic change in the integrated optical and near-infrared spectral energy distributions of galaxies over cosmic time, primarily driven by variations in stellar populations, star formation histories, and dust attenuation.
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2.8K
Authors
700
Institutions
Publications per year
2017–2026
127
Parents
1K
Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
The Astrophysical Journal · 2001 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +16
New Insight on Galaxy Formation and Evolution From Keck Spectroscopy of the Hawaii Deep Fields
L. L. Cowie, A. Songaila, E. M. Hu et al. · The Astronomical Journal · 1996 · 1.6K citations · Full text
Natural Sciences, Astronomy, Physics +15
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700
California Institute of Technology
Pasadena, United States
53 h-index
295 publications
40.3K citations

Space Telescope Science Institute
Baltimore, United States
50 h-index
178 publications
17.2K citations
University of Arizona
Tucson, United States
48 h-index
143 publications
17.9K citations

Johns Hopkins University
Baltimore, United States
48 h-index
209 publications
24.7K citations
University of California, Santa Cruz
Santa Cruz, United States
47 h-index
213 publications
35.3K citations

Durham University
Durham, United Kingdom
43 h-index
133 publications
12.7K citations
European Southern Observatory
Garching bei München, Germany
41 h-index
96 publications
8.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
40 h-index
110 publications
18K citations
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ApJ · 348 publications · 39.8K citations
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243 publications · 17.4K citations
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AJ · 93 publications · 11.5K citations
45
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84 publications · 4.5K citations
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24 publications · 3.1K citations
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