In void environments, the galaxy luminosity function is fitted with Schechter parameters that vary with the void density contrast and the growth function, improving on the McNaught-Roberts model.
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Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
In void environments, the galaxy luminosity function is fitted with Schechter parameters that vary with the void density contrast and the growth function, improving on the McNaught-Roberts model.