4.7 Article

First results from the chara array. II. A description of the instrument

Journal

ASTROPHYSICAL JOURNAL
Volume 628, Issue 1, Pages 453-465

Publisher

IOP PUBLISHING LTD
DOI: 10.1086/430729

Keywords

atmospheric effects; instrumentation : high angular resolution instrumentation : interferometers; techniques : high angular resolution; techniques : interferometric; telescopes

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The CHARA Array is a six 1 m telescope optical/IR interferometric array located on Mount Wilson, California, designed and built by the Center for High Angular Resolution Astronomy of Georgia State University. In this paper we describe the main elements of the Array hardware and software control systems, as well as the data reduction methods currently being used. Our plans for upgrades in the near future are also described.

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