Overview of the Status and Strangeness Capabilities of STAR

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STAR is a large acceptance spectrometer capable of precision measurements of a wide variety of strange particles. We discuss the STAR detector, its configuration during the first two years of RHIC operation, and its initial performance for Au+Au collisions. The expected performance for strangeness physics and initial data on strange particle reconstruction in Au+Au collisions are presented.
Proceedings of the Fifth International Conference on Strangeness in Quark Matter, Berkeley, California, July 20-25, 2000

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