Photometric Sensitivity
Photometric Sensitivity is the minimum detectable flux or radiant power of electromagnetic radiation in specific infrared wavelengths that a space-based infrared observatory can reliably measure, distinguishing it from other observational capabilities by quantifying the instrument's ability to detect weak astronomical sources under given noise conditions.
101
Publications
4.1K
Citations
523
Authors
241
Institutions
Publications per year
2017–2026
13
101
A calculation of confusion noise due to infrared cirrus
III Gautier T. N., F. Boulanger, M. Pérault et al. · The Astronomical Journal · 1992 · 165 citations
Natural Sciences, Astronomy, Physics +17
Photometric Stability of the Lunar Surface
H. H. Kieffer · Icarus · 1997 · 150 citations
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241
Jet Propulsion Laboratory
Pasadena, United States
5 h-index
25 publications
2.5K citations

Space Telescope Science Institute
Baltimore, United States
5 h-index
22 publications
2.2K citations

Johns Hopkins University
Baltimore, United States
4 h-index
11 publications
442 citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
4 h-index
4 publications
66 citations
California Institute of Technology
Pasadena, United States
4 h-index
17 publications
1.1K citations
Institut d'Astrophysique Spatiale
Bures-sur-Yvette, France
4 h-index
36 publications
685 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
3 publications
239 citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
3 h-index
8 publications
856 citations
1–8 of 241
8 publications · 166 citations
8
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6 publications · 201 citations
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6 publications · 243 citations
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JOSA · 6 publications · 411 citations
6
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4 publications · 171 citations
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