Luminosity Function Of Galaxies
The "Luminosity Function of Galaxies" is a statistical model in astrophysics that describes the number density of galaxies per unit luminosity interval, distinguishing it from other galaxy distribution models by quantifying how galaxy populations vary with intrinsic brightness in a given volume of space.
2K
Publications
190.7K
Citations
4.2K
Authors
863
Institutions
Publications per year
2017–2026
264
Variants
Galaxy Luminosity FunctionGlf
Parents
2K
1–5 of 2K
4.2K
31
h-index
29
h-index
26
h-index
25
h-index
24
h-index
1–5 of 4.2K
863
California Institute of Technology
Pasadena, United States
79 h-index
355 publications
53.5K citations

Space Telescope Science Institute
Baltimore, United States
66 h-index
300 publications
51.6K citations

Durham University
Durham, United Kingdom
65 h-index
285 publications
42K citations

Johns Hopkins University
Baltimore, United States
63 h-index
249 publications
37.4K citations

Centre National de la Recherche Scientifique
Paris, France
62 h-index
414 publications
38.9K citations
University of Arizona
Tucson, United States
62 h-index
198 publications
29K citations
European Southern Observatory
Garching bei München, Germany
59 h-index
157 publications
14.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
56 h-index
213 publications
23.8K citations
1–8 of 863
ApJ · 734 publications · 78K citations
140
h-index
514 publications · 48.1K citations
115
h-index
AJ · 178 publications · 20.1K citations
73
h-index
146 publications · 9.3K citations
58
h-index
44 publications · 8.2K citations
32
h-index
1–5