Aperture Photometry
Aperture photometry is a technique in stellar photometry that measures the flux of a celestial source by summing the detected photons within a defined circular or annular aperture centered on the object, while subtracting a local background estimate derived from an adjacent region.
222
Publications
12.3K
Citations
1.6K
Authors
505
Institutions
Publications per year
2017–2026
51
222
Eric Gawiser, Pieter van Dokkum, David Herrera et al. · The Astrophysical Journal Supplement Series · 2006 · 274 citations · Full text
Natural Sciences, Astronomy, Physics +16
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Nanjing Institute of Astronomical Optics & Technology, China
5 publications · 168 citations
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California Institute of Technology
Pasadena, United States
18 h-index
67 publications
4.2K citations

Chinese Academy of Sciences
Beijing, China
14 h-index
57 publications
1.9K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
134 publications
14.8K citations

Space Telescope Science Institute
Baltimore, United States
13 h-index
32 publications
1.8K citations
National Astronomical Observatories
Beijing, China
12 h-index
60 publications
1.5K citations
University of California, Berkeley
Berkeley, United States
12 h-index
26 publications
1.4K citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
30 publications
3.6K citations
University of Chicago
Chicago, United States
11 h-index
29 publications
2.6K citations
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40 publications · 2.3K citations
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AJ · 30 publications · 1.3K citations
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ApJ · 30 publications · 1.4K citations
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29 publications · 1.5K citations
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20 publications · 1.2K citations
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