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Proceedings Paper

Author(s): Harold A. McAlister; William G. Bagnuolo; Theo Armand ten Brummelaar; W. I. Hartkopf; Nils Henning Turner; Allen K. Garrison; William G. Robinson; Stephen T. Ridgway
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Paper 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.

Paper Details

Date Published: 9 June 1994
PDF: 11 pages
Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, (9 June 1994); doi: 10.1117/12.177234
Show Author Affiliations
Harold A. McAlister, CHARA/Georgia State Univ. (United States)
William G. Bagnuolo, CHARA/Georgia State Univ. (United States)
Theo Armand ten Brummelaar, CHARA/Georgia State Univ. (United States)
W. I. Hartkopf, CHARA/Georgia State Univ. (United States)
Nils Henning Turner, CHARA/Georgia State Univ. (United States)
Allen K. Garrison, Georgia Institute of Technology (United States)
William G. Robinson, Georgia Institute of Technology (United States)
Stephen T. Ridgway, National Optical Astronomy Observatories (United States)

Published in SPIE Proceedings Vol. 2200:
Amplitude and Intensity Spatial Interferometry II
James B. Breckinridge, Editor(s)

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