X-ray Luminosity Functions
X-Ray Luminosity Functions is a statistical framework in astrophysics that describes the number density of X-ray-emitting sources per unit luminosity interval, distinguishing itself by quantifying the distribution of X-ray luminosities across populations of extragalactic or Galactic sources to characterize their emission properties and evolution.
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2017–2026
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X-ray Luminosity Function
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The Mass Function of an X‐Ray Flux–limited Sample of Galaxy Clusters
T. H. Reiprich, H. Böhringer · The Astrophysical Journal · 2002 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +15
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Max Planck Institute for Extraterrestrial Physics, Germany
41 publications · 5.8K citations
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
85 h-index
655 publications
59.4K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
80 h-index
739 publications
88.1K citations

Pennsylvania State University
State College, United States
56 h-index
283 publications
25.3K citations

Durham University
Durham, United Kingdom
55 h-index
186 publications
15.5K citations
California Institute of Technology
Pasadena, United States
55 h-index
234 publications
24.7K citations

Centre National de la Recherche Scientifique
Paris, France
53 h-index
495 publications
54.6K citations
Osservatorio astronomico di Bologna
Bologna, Italy
53 h-index
254 publications
31.9K citations
Goddard Space Flight Center
Greenbelt, United States
49 h-index
236 publications
17.2K citations
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ApJ · 777 publications · 62.8K citations
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501 publications · 36.8K citations
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236 publications · 18.8K citations
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40 publications · 5.2K citations
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AJ · 68 publications · 3.8K citations
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