Distance-redshift Relation
The Distance-Redshift Relation is a theoretical framework in cosmology that specifies the quantitative dependence of the proper distance to a celestial object on its cosmological redshift, uniquely encoding the expansion history of the universe through the integral of the inverse Hubble parameter over redshift.
700
Publications
54K
Citations
1.6K
Authors
623
Institutions
Publications per year
2017–2026
173
Parents
700
In the realm of the Hubble tension—a review of solutions <sup>*</sup>
Classical and Quantum Gravity · 2021 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 700
1.6K
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623
University of California, Berkeley
Berkeley, United States
27 h-index
52 publications
9.8K citations
University of Chicago
Chicago, United States
26 h-index
55 publications
13.5K citations

Centre National de la Recherche Scientifique
Paris, France
25 h-index
120 publications
22.4K citations
California Institute of Technology
Pasadena, United States
21 h-index
44 publications
8.7K citations
University of Arizona
Tucson, United States
21 h-index
40 publications
5.6K citations
The University of Tokyo
Tokyo, Japan
18 h-index
37 publications
5.1K citations

Lawrence Berkeley National Laboratory
Berkeley, United States
18 h-index
45 publications
13.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
31 publications
7.7K citations
1–8 of 623
ApJ · 136 publications · 11.4K citations
60
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101 publications · 12K citations
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JCAP · 70 publications · 3.4K citations
36
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49 publications · 3.4K citations
32
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PRD · 31 publications · 1.4K citations
24
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