Paper
9 June 1994 CHARA Array
Author Affiliations +
Abstract
The CHARA array is an optical and IR imaging array of seven 1-m aperture telescopes with a Y-shaped configuration contained within a 400-m diameter circle. The facility will be capable of submilliarcsecond imaging and will be devoted to a broad program of science aimed at fundamental stellar astrophysics in the visible and the astrophysics of young stellar objects in the infrared spectral regions. The concept for the array has been carried through Phase A feasibility and Phase B preliminary design stages with funding provided by the National Science Foundation. This paper will provide a progress report on the status of the project.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Harold A. McAlister, William G. Bagnuolo Jr., Theo Armand ten Brummelaar, W. I. Hartkopf, Nils Henning Turner, Allen K. Garrison, William G. Robinson, and Stephen T. Ridgway "CHARA Array", Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, (9 June 1994); https://doi.org/10.1117/12.177234
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Cited by 8 scholarly publications.
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KEYWORDS
Telescopes

Adaptive optics

Interferometry

Infrared imaging

Stars

Visibility

Visible radiation

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