Open Cluster Luminosity Function
Open Cluster Luminosity Function is a statistical construct that characterizes the distribution of absolute magnitudes among open star clusters in a given region of the sky, serving to quantify the number of clusters per unit luminosity interval as a function of brightness.
98
Publications
4.9K
Citations
199
Authors
132
Institutions
Publications per year
2017–2026
9
Parents
98
CCD photometry of the old open cluster M67
Kent A. Montgomery, Laurence A. Marschall, K. A. Janes · The Astronomical Journal · 1993 · 296 citations · Full text
Natural Sciences, Astronomy, Physics +17
A deep imaging survey of the Pleiades with ROSAT
J. R. Stauffer, J. P. Caillault, Marc Gagné et al. · The Astrophysical Journal Supplement Series · 1994 · 206 citations
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Aryabhatta Research Institute of Observational Sciences, India
5 publications · 159 citations
5
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4
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4
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1–5 of 199
132
Osservatorio Astronomico di Padova
Padua, Italy
10 h-index
27 publications
597 citations

University of Padua
Padua, Italy
7 h-index
15 publications
365 citations
Universidade Federal do Rio Grande do Sul
Porto Alegre, Brazil
6 h-index
13 publications
550 citations
Heidelberg University
Heidelberg, Germany
6 h-index
18 publications
660 citations
Main Astronomical Observatory
Kyiv, Ukraine
5 h-index
5 publications
201 citations

University of Edinburgh
Edinburgh, United Kingdom
4 h-index
5 publications
283 citations
Institute of Astronomy
Moscow, Russia
4 h-index
11 publications
292 citations

University of Leicester
Leicester, United Kingdom
4 h-index
8 publications
217 citations
1–8 of 132
20 publications · 882 citations
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AJ · 18 publications · 1.3K citations
17
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ApJ · 15 publications · 1.2K citations
14
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16 publications · 626 citations
14
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3 publications · 46 citations
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