Photometric Zero Points
Photometric Zero Points is a calibration constant in stellar photometry that defines the magnitude of a source producing one detected photon per unit time at a specified wavelength or passband, thereby establishing the reference flux level for photometric measurements in ultraviolet photometry and related observational systems.
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7.6K
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312
Authors
147
Institutions
Publications per year
2017–2026
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The Sloan Digital Sky Survey Photometric System
M. Fukugita, Takashi Ichikawa, James E. Gunn et al. · The Astronomical Journal · 1996 · 3.1K citations · Full text
Photometric calibration of the Swift ultraviolet/optical telescope
T. Poole, A. A. Breeveld, M. J. Page et al. · Monthly Notices of the Royal Astronomical Society · 2007 · 969 citations · Full text
Natural Sciences, Astronomy, Physics +17
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147

Australian National University
Canberra, Australia
5 h-index
6 publications
590 citations
Princeton University
Princeton, United States
5 h-index
12 publications
5.6K citations
Millennium Institute of Astrophysics
Santiago, Chile
4 h-index
7 publications
201 citations
University of Southampton
Southampton, United Kingdom
3 h-index
3 publications
369 citations
Yale University
New Haven, United States
3 h-index
9 publications
266 citations

Pennsylvania State University
State College, United States
3 h-index
13 publications
11.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
3 h-index
3 publications
454 citations
NSF NOIRLab
Tucson, United States
3 h-index
10 publications
386 citations
1–8 of 147
AJ · 9 publications · 3.6K citations
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PASP · 7 publications · 385 citations
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6 publications · 1.4K citations
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ApJ · 4 publications · 326 citations
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4 publications · 1.3K citations
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