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Published online by Cambridge University Press: 07 August 2017
Our aim is to quantify the stellar population within the nuclear regions of AGN by means of long slit spectroscopic observations in the optical range (5000-10000Å), including MgI, NaI, TiO, CN, CaIIT. We wish to determine whether there is a relationship between central activity and stellar population, and to determine the nature of the featureless continuum.