A Method for Obtaining the Nuclear Component in Active Galaxies |
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| Authors: | Miguel Sanchez Portal Angeles I Diaz Beltran |
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| Affiliation: | (1) Dpto. de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049- Madrid, Spain;;(2) LAEFF/INTA, P.O. Box 50727, 28080- Madrid, Spain |
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| 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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