Radio Luminosity Functions is a statistical construct in extragalactic radio astronomy that describes the number density of radio sources per unit luminosity interval, distinguishing it from other luminosity functions by its specific application to continuum emission from extragalactic radio sources across cosmic time.
731
Publications
54.5K
Citations
1.9K
Authors
568
Institutions
Publications per year
2017–2026
114
Publications
731
P. N. Best, Guinevere Kauffmann, Timothy M. Heckman et al. · Monthly Notices of the Royal Astronomical Society · 2005 · 774 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 731
Authors
1.9K
- HJ
20
h-index
- MJ
16
h-index
- SR
16
h-index
- MJ
15
h-index
- JJ
14
h-index
1–5 of 1.9K
Institutions
568
National Radio Astronomy Observatory
Charlottesville, United States
39 h-index
94 publications
11.1K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
33 h-index
84 publications
4.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
32 h-index
74 publications
6.5K citations
Royal Observatory
Edinburgh, United Kingdom
32 h-index
78 publications
8.9K citations
Leiden University
Leiden, The Netherlands
29 h-index
76 publications
6.9K citations
University of Oxford
Oxford, United Kingdom
28 h-index
90 publications
8K citations
California Institute of Technology
Pasadena, United States
27 h-index
137 publications
10.2K citations
University of Cambridge
Cambridge, United Kingdom
24 h-index
51 publications
3.8K citations
1–8 of 568
Venues
- Monthly Notices of the Royal Astronomical Society
247 publications · 22K citations
72
h-index
- The Astrophysical Journal
ApJ · 200 publications · 16.8K citations
69
h-index
- Astronomy and Astrophysics
51 publications · 2.9K citations
31
h-index
- The Astronomical Journal
AJ · 47 publications · 2.9K citations
29
h-index
- The Astrophysical Journal Supplement Series
19 publications · 2.2K citations
19
h-index
1–5