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

被引：461

作者：

ten Brummelaar, TA ^{[1
]}

McAlister, HA

Ridgway, ST

Bagnuolo, WG

Turner, NH

Sturmann, L

Sturmann, J

Berger, DH

Ogden, CE

Cadman, R

Hartkopf, WI

Hopper, CH

Shure, MA

机构：

[1] Mt Wilson Observ, CHARA Array, Mt Wilson, CA 91023 USA

[2] Georgia State Univ, Ctr High Angular Resolut Astron, Atlanta, GA 30302 USA

[3] Natl Opt Astron Observ, Kitt Peak Natl Observ, Tucson, AZ 85726 USA

[4] Georgia State Univ, Dept Phys & Astron, Atlanta, GA 30302 USA

来源：

ASTROPHYSICAL JOURNAL | 2005年 / 628卷 / 01期

关键词：

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

D O I：

10.1086/430729

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：453 / 465

页数：13

共 43 条

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