Photometric Transformations
Photometric Transformations is a methodological framework in stellar photometry that enables the conversion of observed magnitudes and color indices from one photometric system to another by accounting for differences in instrumental response functions, atmospheric extinction, and standardization conventions.
127
Publications
20.8K
Citations
447
Authors
235
Institutions
Publications per year
2017–2026
21
Variants
Photometric Transformation
127
M. S. Bessell · Publications of the Astronomical Society of the Pacific · 1990 · 1.2K citations
Natural Sciences, Astronomy, Physics +16
The u'g'r'i'z' Standard-Star System
J. A. Smith, D. L. Tucker, S. Kent et al. · 2002 · 1.1K citations
Natural Sciences, Astronomy, Physics +17
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235

Australian National University
Canberra, Australia
9 h-index
18 publications
5.1K citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
16 publications
482 citations

Space Telescope Science Institute
Baltimore, United States
6 h-index
8 publications
983 citations
Osservatorio Astronomico di Padova
Padua, Italy
4 h-index
4 publications
576 citations

Mount Stromlo Observatory
Canberra, Australia
4 h-index
7 publications
5.6K citations

Chinese Academy of Sciences
Beijing, China
4 h-index
15 publications
1.4K citations
University of Cambridge
Cambridge, United Kingdom
4 h-index
28 publications
2.1K citations
Princeton University
Princeton, United States
4 h-index
4 publications
3.3K citations
1–8 of 235
PASP · 18 publications · 6.5K citations
15
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AJ · 15 publications · 2.2K citations
14
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10 publications · 876 citations
10
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ApJ · 9 publications · 1.7K citations
9
h-index
6 publications · 1.3K citations
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