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Published online by Cambridge University Press: 25 May 2016
In Dravskikh & Dravskikh (1996) the results of a statistical analysis of quasar luminosity as a function of redshift, if it is assumed to be cosmological, are given (see Fig.1). Three quasar samples were analyzed separately:
• quasars with absorption lines;
• quasars associated with galaxies or association-quasars not having absorption lines (from Burbidge et al. 1996);
• other quasars not included in the first two groups.