Stellar Photometry
Stellar Photometry is the scientific measurement of the brightness or flux of stars, distinguished by its focus on quantifying stellar light intensity across specific wavelength bands to determine physical properties such as luminosity, temperature, and distance.
6.8K
Publications
470.9K
Citations
16.2K
Authors
1.9K
Institutions
Publications per year
2017–2026
1.1K
6.8K
A. G. A. Brown, A. Vallenari, T. Prusti et al. · Astronomy and Astrophysics · 2018 · 8.7K citations · Full text
Natural Sciences, Astronomy, Physics +15
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1.9K

Space Telescope Science Institute
Baltimore, United States
114 h-index
952 publications
136.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
108 h-index
1K publications
184.3K citations

Centre National de la Recherche Scientifique
Paris, France
104 h-index
2.5K publications
923K citations
California Institute of Technology
Pasadena, United States
100 h-index
1.1K publications
128.3K citations
University of Arizona
Tucson, United States
90 h-index
625 publications
65.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
81 h-index
677 publications
206.1K citations

Sorbonne Université
Paris, France
79 h-index
770 publications
257.5K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
77 h-index
707 publications
51.2K citations
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ApJ · 1.3K publications · 98.3K citations
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AJ · 1.1K publications · 86.5K citations
127
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932 publications · 67.4K citations
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1.2K publications · 56.7K citations
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276 publications · 36.6K citations
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