Point Spread Function Modeling
Point Spread Function Modeling is a computational and mathematical framework in astrometric and imaging sciences that characterizes the spatial response of an optical or detector system to a point source by modeling the diffraction, aberration, and noise processes that determine the observed image profile, distinguishing it from general image formation models through its focus on system-specific and environment-induced blurring mechanisms.
492
Publications
23K
Citations
1.8K
Authors
725
Institutions
Publications per year
2017–2026
89
492
1–5 of 492
1.8K
Space Telescope Science Institute, United States
5 publications · 784 citations
5
h-index
5
h-index
5
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5
h-index
4
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1–5 of 1.8K
725

Centre National de la Recherche Scientifique
Paris, France
20 h-index
85 publications
5.1K citations

Space Telescope Science Institute
Baltimore, United States
15 h-index
46 publications
4.5K citations
California Institute of Technology
Pasadena, United States
13 h-index
28 publications
1.5K citations
CEA Paris-Saclay
Gif-sur-Yvette, France
12 h-index
33 publications
2.5K citations
University of Arizona
Tucson, United States
12 h-index
33 publications
1.1K citations
Stanford University
Stanford, United States
12 h-index
86 publications
6.4K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
12 h-index
35 publications
3.3K citations
Jet Propulsion Laboratory
Pasadena, United States
11 h-index
19 publications
1.1K citations
1–8 of 725
31 publications · 2.2K citations
21
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25 publications · 1.3K citations
20
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35 publications · 1.7K citations
18
h-index
15 publications · 1.1K citations
15
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ApJ · 15 publications · 902 citations
14
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1–5