Towards the Luminosity Function of Seyfert Galaxy Nuclei
The optical and radio luminosity functions of Seyfert galaxies for total emission of the systems are briefly reviewed. A project of CCD-photometry aimed at determining a luminosity function for Seyfert nuclei is described. The merits of integrated and nuclear magnitudes with respect to Seyfert luminosity functions are discussed. Finally, a few remarks on systematic survey incompletenesses are made.
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