White Dwarf Luminosity Function
The White Dwarf Luminosity Function is a statistical representation that quantifies the number density of white dwarf stars per unit luminosity interval, serving as a fundamental diagnostic tool in stellar population studies to constrain the age, formation history, and evolution of galactic stellar populations.
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297
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Wdlf
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An independent method for determining the age of the universe
D. E. Winget, C. Hansen, James Liebert et al. · The Astrophysical Journal · 1987 · 426 citations · Full text
Natural Sciences, Astronomy, Physics +11
A COMPREHENSIVE SPECTROSCOPIC ANALYSIS OF DB WHITE DWARFS
The Astrophysical Journal · 2011 · 355 citations · Full text
Natural Sciences, Astronomy, Physics +17
The luminosity function of white dwarfs
James Liebert, C. C. Dahn, D. G. Monet · The Astrophysical Journal · 1988 · 283 citations
Natural Sciences, Astronomy, Physics +13
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Universitat Politècnica de Catalunya
Barcelona, Spain
23 h-index
69 publications
2.9K citations
Institut d'Estudis Espacials de Catalunya
Castelldefels, Spain
23 h-index
83 publications
4.6K citations
Institute of Space Sciences
Cerdanyola del Vallès, Spain
15 h-index
22 publications
2K citations
Instituto de Astrofísica de La Plata
La Plata, Argentina
13 h-index
22 publications
1.7K citations

Consejo Nacional de Investigaciones Científicas y Técnicas
Buenos Aires, Argentina
13 h-index
22 publications
1.7K citations

Universidad Nacional de La Plata
La Plata, Argentina
13 h-index
21 publications
1.6K citations
University of Arizona
Tucson, United States
10 h-index
13 publications
2.7K citations

University of British Columbia
Vancouver, Canada
9 h-index
29 publications
3.5K citations
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ApJ · 64 publications · 5.7K citations
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28 publications · 1.7K citations
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14 publications · 445 citations
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AJ · 9 publications · 490 citations
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PASP · 5 publications · 69 citations
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