Infrared Luminosity Functions
Infrared Luminosity Functions is a statistical construct in extragalactic infrared astronomy that describes the number density of galaxies per unit comoving volume per unit infrared luminosity interval, distinguishing it from related luminosity-based distributions by specifically quantifying the galaxy population's infrared-emitting properties as a function of luminosity.
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Infrared Luminosity Function
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New Insight on Galaxy Formation and Evolution From Keck Spectroscopy of the Hawaii Deep Fields
L. L. Cowie, A. Songaila, E. M. Hu et al. · The Astronomical Journal · 1996 · 1.6K citations · Full text
Natural Sciences, Astronomy, Physics +15
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France
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California Institute of Technology
Pasadena, United States
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Centre National de la Recherche Scientifique
Paris, France
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213 publications
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University of Arizona
Tucson, United States
36 h-index
161 publications
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Infrared Processing and Analysis Center
Pasadena, United States
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92 publications
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
32 h-index
89 publications
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Kitt Peak National Observatory
Tucson, United States
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CEA Paris-Saclay
Gif-sur-Yvette, France
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
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ApJ · 214 publications · 21.6K citations
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AJ · 43 publications · 4.5K citations
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