Globular Cluster Luminosity Function
Globular Cluster Luminosity Function is a statistical model that describes the distribution of luminosities of globular clusters in a galaxy, serving as a standard candle method for estimating extragalactic distances based on the characteristic peak in their brightness distribution.
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38K
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388
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Publications per year
2017–2026
46
Variants
Gclf
Parents
581
A Catalog of Parameters for Globular Clusters in the Milky Way
William E. Harris · The Astronomical Journal · 1996 · 4.6K citations
Natural Sciences, Astronomy, Physics +17
Properties of stellar generations in globular clusters and relations with global parameters
E. Carretta, A. Bragaglia, R. Gratton et al. · Astronomy and Astrophysics · 2010 · 522 citations · Full text
Natural Sciences, Astronomy, Physics +17
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European Southern Observatory
Garching bei München, Germany
38 h-index
77 publications
5.3K citations

Space Telescope Science Institute
Baltimore, United States
34 h-index
98 publications
10K citations
University of California, Santa Cruz
Santa Cruz, United States
29 h-index
61 publications
5.9K citations
Herzberg Institute of Astrophysics
Victoria, Canada
28 h-index
59 publications
4.9K citations

McMaster University
Hamilton, Canada
24 h-index
55 publications
3.8K citations
California Institute of Technology
Pasadena, United States
23 h-index
48 publications
4.6K citations
Osservatorio astronomico di Bologna
Bologna, Italy
21 h-index
73 publications
6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
21 h-index
41 publications
3.4K citations
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ApJ · 190 publications · 11.4K citations
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AJ · 129 publications · 12.8K citations
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86 publications · 4.9K citations
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40 publications · 2.1K citations
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14 publications · 1.1K citations
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