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INTRODUCTION

In Paper I, by comparing the FBS (Markarian et al. 1989) and BQS (Green et al. 1986) surveys in their area in common, we derived a completeness of $\sim$70% for the BQS. A number of bright AGNs have since been discovered in the area which, together with our new spectroscopic observations, allowed us to refine our previous estimate of the BQS completeness.




7/28/2000