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A Method for Obtaining the Nuclear Component in Active Galaxies
Authors:Miguel Sanchez Portal  Angeles I Diaz Beltran
Institution:(1) Dpto. de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049- Madrid, Spain;;(2) LAEFF/INTA, P.O. Box 50727, 28080- Madrid, Spain
Abstract:We present a new method for the obtention of the nuclear component of active galatic nuclei, that relies on the convolution of a two-dimensional model of the host galaxy, based on seeing-free morphological parameters, with the seeing PSF. The procedure overcomes some limitations of the methods currently in use and does not assume that the nucleus is unresolved. This revised version was published online in July 2006 with corrections to the Cover Date.
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