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THE ASTROPHYSICAL JOURNAL, 503 : 617 631, 1998 August 20 (1998. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE GALAXY LUMINOSITY FUNCTION AT z 0.05 : DEPENDENCE ON MORPHOLOGY
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Form galaxy luminosity function is a form used to measure the distribution of galaxy luminosities in a given region of space.
Any professional or organization conducting research or studying galaxies is required to file form galaxy luminosity function.
To fill out form galaxy luminosity function, you need to provide information about the observed galaxies, their luminosities, and the specific region of space being studied. You may also need to provide details about the methodology used to calculate the luminosity function.
The purpose of form galaxy luminosity function is to gather data on the distribution of galaxy luminosities, which can be used to study the evolution of galaxies, their formation processes, and the overall structure of the universe.
On form galaxy luminosity function, you must report the observed galaxy luminosities, the specific region of space being studied, and any relevant details about the methodology used for calculation.
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