Point Spread Function Photometry
Point Spread Function Photometry is a photometric method that models the spatial distribution of stellar light as a mathematical point spread function to achieve precise flux measurements by fitting the expected instrumental response to observed point-source images in ultraviolet and stellar photometry.
84
Publications
11.8K
Citations
546
Authors
299
Institutions
Publications per year
2017–2026
26
84
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546
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299

Space Telescope Science Institute
Baltimore, United States
13 h-index
32 publications
5.2K citations

Centre National de la Recherche Scientifique
Paris, France
10 h-index
31 publications
1K citations
Université Bourgogne Franche-Comté
Besançon, France
8 h-index
16 publications
781 citations
European Southern Observatory
Garching bei München, Germany
7 h-index
9 publications
252 citations
Heidelberg University
Heidelberg, Germany
6 h-index
10 publications
1.1K citations

Johns Hopkins University
Baltimore, United States
6 h-index
9 publications
690 citations
California Institute of Technology
Pasadena, United States
6 h-index
32 publications
1.5K citations

Kitt Peak National Observatory
Tucson, United States
6 h-index
9 publications
1.8K citations
1–8 of 299
17 publications · 918 citations
15
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ApJ · 14 publications · 902 citations
13
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AJ · 11 publications · 552 citations
11
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PASP · 10 publications · 7.1K citations
10
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9 publications · 246 citations
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1–5