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Published online by Cambridge University Press: 25 May 2016
George Djorgovski's message to me on behalf of the organizing committee suggested that I discuss 1) Evolution of the Quasar Luminosity Function; 2) Possible Differences among Radio-Loud, Radio-Quiet, and X-Ray Selected Samples; 3) Quasars as Probes of Clustering and Large-Scale Structure at High Redshift; 4) Searches for Extremely Distant Quasars; 5) Theoretical Implications; 6) Major Surveys in Progress and Planned; and 7) What Surveys Should We Do in the Future. To cover all these topics in a 25-minute talk and 7-page article is a challenge, but I am happy to try.