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Proceedings Paper

CHARA recent technology and science
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Paper Abstract

Georgia State University's Center for High Angular Resolution Astronomy (CHARA) operates a multi-telescope, long-baseline, optical/infrared interferometric array on Mt. Wilson, California. We present an update on the status of this facility along with a sample of preliminary results from current scientific programs.

Paper Details

Date Published: 20 October 2004
PDF: 10 pages
Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); doi: 10.1117/12.551697
Show Author Affiliations
Harold A. McAlister, Georgia State Univ. (United States)
Theo A. ten Brummelaar, Georgia State Univ. (United States)
Jason P. Aufdenberg, National Optical Astronomy Observatory (United States)
William G. Bagnuolo, Georgia State Univ. (United States)
David H. Berger, Georgia State Univ. (United States)
Vincent Coude du Foresto, LESIA, Observatoire de Paris-Meudon (France)
Antoine Merand, LESIA, Observatoire de Paris-Meudon (France)
Chad Ogden, Georgia State Univ. (United States)
Stephen T. Ridgway, Georgia State Univ. (United States)
National Optical Astonomy Observatory (United States)
LESIA, Observatoire de Paris-Meudon (France)
Judit Sturmann, Georgia State Univ. (United States)
Laszlo Sturmann, Georgia State Univ. (United States)
Stuart Taylor, Georgia State Univ. (United States)
Nils H. Turner, Georgia State Univ. (United States)


Published in SPIE Proceedings Vol. 5491:
New Frontiers in Stellar Interferometry
Wesley A. Traub, Editor(s)

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