Stellar Spectral Classification
Stellar Spectral Classification is a systematic astrophysical framework that categorizes stars based on their electromagnetic spectra, particularly the patterns of absorption lines, to infer fundamental physical properties such as temperature, luminosity, and chemical composition.
1.3K
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3.5K
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821
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Publications per year
2017–2026
183
1.3K
Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
Iskra Strateva, Željko Ivezić, G. R. Knapp et al. · The Astronomical Journal · 2001 · 1.6K citations · Full text
Natural Sciences, Astronomy, Physics +13
SEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH<i>g</i>= 14-20
B. Yanny, Constance M. Rockosi, Heidi Jo Newberg et al. · The Astronomical Journal · 2009 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +17
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California Institute of Technology
Pasadena, United States
45 h-index
131 publications
20.8K citations

Centre National de la Recherche Scientifique
Paris, France
36 h-index
209 publications
14.9K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
34 h-index
114 publications
9.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
32 h-index
103 publications
11.8K citations
University of California, Berkeley
Berkeley, United States
31 h-index
106 publications
17K citations

Space Telescope Science Institute
Baltimore, United States
31 h-index
66 publications
7.7K citations
National Astronomical Observatories
Beijing, China
30 h-index
355 publications
13.8K citations

Chinese Academy of Sciences
Beijing, China
29 h-index
267 publications
9.3K citations
1–8 of 821
ApJ · 298 publications · 20.8K citations
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AJ · 170 publications · 18.4K citations
60
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115 publications · 18.2K citations
57
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158 publications · 9.2K citations
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167 publications · 8.2K citations
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