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Published online by Cambridge University Press: 19 July 2016
The merits of selecting samples of quasars for statistical analysis on the basis of optical variability is discussed. Samples selected this way are essentially uncontaminated by spurious objects, and contain no serious redshift biasses. A preliminary sample from a long term survey suggests a timescale of variation for quasars of about four years, and indicates a fall off in numbers at around B = 20.