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The Morphological Luminosity Function
1988We obtain the morphological luminosity function for galaxies assuming that they form at high density regions of a filtered Gaussian random field. We compare our results with some observations of the LF for E and E+SO galaxies. Using scale-free spectra, we obtain bell-shaped curves that follow the observations.
J. L. Sanz, E. Martínez-González
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The radio luminosity function and the luminosity diameter function of extragalactic radio sources
Astronomische Nachrichten, 1971AbstractOn the basis of a radio index‐surface brightness diagram recently published, the luminosity function and the luminosity diameter function are obtained. The uncertainties due to the incompleteness of the sample are of the same order as the statistical uncertainties.
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The Quasar Luminosity Function
1993Recent work on the quasar luminosity function at radio, optical and X-ray wavelengths is reviewed. It is demonstrated that the evolution of the quasar luminosity function in all three regimes is marked by a strong and approximately similar power-law increase in luminosity, L ∝ (1 + z) 3±0.5, between the present epoch and z ≈ 2.
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On the FRB luminosity function – – II. Event rate density
Monthly Notices of the Royal Astronomical Society, 2020Wei-Yang Wang, Rui Luo
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The ALMA REBELS Survey: the first infrared luminosity function measurement at z ∼ 7
Monthly Notices of the Royal Astronomical Society, 2023Pascal Oesch +2 more
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The Durham/UKST Galaxy Redshift Survey - II. The field galaxy luminosity function
Monthly Notices of the Royal Astronomical Society, 1998Tom Shanks, R Fong, Q A Parker
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The Faint End of the Stellar Luminosity Function
Annual Review of Astronomy and Astrophysics, 1993Michael Bessell, Guy Stringfellow
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Deriving an X-ray luminosity function of dwarf novae based on parallax measurements
Monthly Notices of the Royal Astronomical Society, 2010J R Thorstensen
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