Point Spread Function Fitting
Point Spread Function Fitting is a computational method in differential astrometry that models the spatial distribution of light from a point source by matching an empirical or theoretical point spread function to observed image data to precisely determine the source's position and photometric properties.
132
Publications
12.4K
Citations
755
Authors
325
Institutions
Publications per year
2017–2026
30
132
The Second Data Release of the Sloan Digital Sky Survey
Kevork N. Abazajian, Jennifer Adelman-McCarthy, Marcel A. Agüeros et al. · The Astronomical Journal · 2004 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +17
STRUCTURAL PARAMETERS OF GALAXIES IN CANDELS
Arjen van der Wel, Eric F. Bell, Elizabeth J. McGrath et al. · The Astrophysical Journal Supplement Series · 2012 · 551 citations · Full text
Natural Sciences, Astronomy, Physics +14
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325

Space Telescope Science Institute
Baltimore, United States
9 h-index
28 publications
9K citations
Princeton University
Princeton, United States
9 h-index
28 publications
19.2K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
7 h-index
14 publications
906 citations
CEA Paris-Saclay
Gif-sur-Yvette, France
7 h-index
14 publications
906 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
16 publications
368 citations
Stanford University
Stanford, United States
7 h-index
18 publications
1.3K citations
University of Pennsylvania
Philadelphia, United States
6 h-index
15 publications
2.9K citations
Jet Propulsion Laboratory
Pasadena, United States
6 h-index
9 publications
660 citations
1–8 of 325
ApJ · 14 publications · 538 citations
13
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13 publications · 1.2K citations
12
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AJ · 14 publications · 1.5K citations
12
h-index
12 publications · 530 citations
11
h-index
7 publications · 1.1K citations
7
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