Resolved Source Counts
Resolved Source Counts is a methodological construct in observational astrophysics that refers to the statistical enumeration of individually detected infrared-emitting celestial sources contributing to the Cosmic Infrared Background, distinguished by their angular resolution and flux density measurements from deep-field surveys.
18
Publications
1.8K
Citations
119
Authors
78
Institutions
Publications per year
2017–2026
3
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H. Dole, G. Lagache, Jean-Loup Puget et al. · CERN Document Server (European Organization for Nuclear Research) · 2006 · 292 citations · Full text
Natural Sciences, Astronomy, Physics +15
Structural properties of the M31 dwarf spheroidal galaxies
2005 · 160 citations
Natural Sciences, Astronomy, Physics +15
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California Institute of Technology
Pasadena, United States
4 h-index
8 publications
742 citations
University of California, Los Angeles
Los Angeles, United States
3 h-index
3 publications
327 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
3 h-index
16 publications
2.8K citations
Osservatorio astronomico di Bologna
Bologna, Italy
2 h-index
2 publications
364 citations

Space Telescope Science Institute
Baltimore, United States
2 h-index
2 publications
267 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
2 h-index
4 publications
728 citations
Harvard University
Cambridge, United States
2 h-index
16 publications
2.8K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
2 h-index
2 publications
84 citations
1–8 of 78
ApJ · 4 publications · 148 citations
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3 publications · 276 citations
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Repository · 2 publications · 303 citations
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2 publications · 183 citations
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2 publications · 517 citations
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