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In spite of the almost all-encompassing variability of Be stars, surveys playa steadily increasing role in complementing the insights gained fromsingle-star studies. The definition of classical Be stars as recently augmentedby \cite{Rivinius2013} enables unambiguous identification of Be stars in a muchincreased range of observations. Results of targeted surveys are brieflyreviewed for the effects of metallicity, binarity, and evolution. It stillremains to be seen whether Be stars are safe benchmarks for the calibration ofevolutionary models with rapid rotation.

Be Stars as Seen Through Telescopes in Survey Mode (I)