Mass Function Of Galaxies
The Mass Function of Galaxies is a statistical construct in astrophysics that describes the number density of galaxies per unit comoving volume as a function of their stellar or total mass, distinguishing it from other galaxy distribution measures by quantifying the abundance of galaxies across the mass spectrum.
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32.6K
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922
Authors
348
Institutions
Publications per year
2017–2026
52
Variants
Galaxy Mass Function
Parents
260
HIGH-RESOLUTION ROTATION CURVES AND GALAXY MASS MODELS FROM THINGS
The Astronomical Journal · 2008 · 924 citations · Full text
Natural Sciences, Astronomy, Physics +14
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348

Centre National de la Recherche Scientifique
Paris, France
20 h-index
79 publications
33.9K citations
Max Planck Institute for Astrophysics
Garching, Germany
20 h-index
44 publications
13.2K citations
Leiden University
Leiden, The Netherlands
18 h-index
37 publications
6.3K citations
European Southern Observatory
Garching bei München, Germany
18 h-index
24 publications
6.6K citations
Swinburne University of Technology
Melbourne, Australia
18 h-index
36 publications
3.3K citations

Trieste Astronomical Observatory
Trieste, Italy
17 h-index
39 publications
3.8K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
17 h-index
29 publications
7.4K citations

University of Massachusetts Amherst
Amherst Center, United States
17 h-index
27 publications
11.1K citations
1–8 of 348
90 publications · 9.9K citations
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ApJ · 82 publications · 8.6K citations
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16 publications · 3K citations
15
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AJ · 9 publications · 2.3K citations
9
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6 publications · 573 citations
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