The immediate goal of modern observational astronomy is to monitor continuously the position and brightness of all objects in the sky brighter than ∼24th magnitude. This review describes wide‐field telescopes designed for this task – both existing and planned. Many systems are described for the first time (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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V. Yu. Terebizh (2011) studied this question.
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