Survey Depth
Survey Depth is a metric in survey astronomy that quantifies the faintest apparent magnitude of celestial objects detectable by a given sky survey, distinguishing it from other survey characteristics by its focus on sensitivity limits rather than spatial coverage or resolution.
73
Publications
4.8K
Citations
728
Authors
316
Institutions
Publications per year
2017–2026
21
Variants
Limiting Magnitude
Parents
73
The skewness of the aperture mass statistic
Monthly Notices of the Royal Astronomical Society · 2004 · 311 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 73
728
Kavli Institute for Particle Astrophysics and Cosmology, United States
4 publications · 475 citations
4
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4
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4
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3
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3
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1–5 of 728
316
University of Cambridge
Cambridge, United Kingdom
9 h-index
21 publications
2K citations
Kavli Institute for Particle Astrophysics and Cosmology
Menlo Park, United States
8 h-index
36 publications
4.3K citations
Leiden University
Leiden, The Netherlands
8 h-index
12 publications
698 citations
Stanford University
Stanford, United States
7 h-index
31 publications
3.7K citations
SLAC National Accelerator Laboratory
Menlo Park, United States
6 h-index
25 publications
3.3K citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
9 publications
1K citations
The Ohio State University
Columbus, United States
6 h-index
16 publications
1.6K citations
University of Oxford
Oxford, United Kingdom
6 h-index
11 publications
239 citations
1–8 of 316
ApJ · 14 publications · 1.1K citations
13
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13 publications · 973 citations
13
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5 publications · 297 citations
5
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3 publications · 444 citations
3
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PASA · 2 publications · 259 citations
2
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1–5