Galaxy Bias
Galaxy Bias is a theoretical construct in cosmology that quantifies the difference between the spatial distribution of galaxies and the underlying dark matter density field, serving as a proportionality factor that relates fluctuations in galaxy number counts to matter overdensities on large scales.
770
Publications
60.4K
Citations
2.2K
Authors
576
Institutions
Publications per year
2017–2026
225
Variants
Galaxy Bias Factor
770
1–5 of 770
2.2K
24
h-index
24
h-index
22
h-index
20
h-index
19
h-index
1–5 of 2.2K
576
Princeton University
Princeton, United States
49 h-index
148 publications
23.8K citations
University of Chicago
Chicago, United States
42 h-index
168 publications
14.5K citations

University of Edinburgh
Edinburgh, United Kingdom
41 h-index
120 publications
11.3K citations
The Ohio State University
Columbus, United States
41 h-index
130 publications
13.9K citations
University of Portsmouth
Portsmouth, United Kingdom
39 h-index
165 publications
14.4K citations
University of California, Berkeley
Berkeley, United States
38 h-index
92 publications
7.5K citations
California Institute of Technology
Pasadena, United States
38 h-index
109 publications
11.1K citations

Lawrence Berkeley National Laboratory
Berkeley, United States
36 h-index
88 publications
7.4K citations
1–8 of 576
262 publications · 18.5K citations
74
h-index
ApJ · 159 publications · 17K citations
66
h-index
JCAP · 82 publications · 5K citations
38
h-index
46 publications · 5.8K citations
33
h-index
PRD · 29 publications · 1.8K citations
24
h-index
1–5