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Proceedings Paper

Recent progress at the CHARA interferometric array
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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 a brief update on the status of this facility along with summaries of the first scientific results from the Array.

Paper Details

Date Published: 27 June 2006
PDF: 7 pages
Proc. SPIE 6268, Advances in Stellar Interferometry, 62680G (27 June 2006); doi: 10.1117/12.671811
Show Author Affiliations
H. A. McAlister, Ctr. for High Angular Resolution Astronomy, Georgia State Univ. (United States)
T. A. ten Brummelaar, Ctr. for High Angular Resolution Astronomy, Georgia State Univ. (United States)
L. Sturmann, Ctr. for High Angular Resolution Astronomy, Georgia State Univ. (United States)
J. Sturmann, Ctr. for High Angular Resolution Astronomy, Georgia State Univ. (United States)
N. H. Turner, Ctr. for High Angular Resolution Astronomy, Georgia State Univ. (United States)
S. T. Ridgway, National Optical Astronomy Observatories (United States)


Published in SPIE Proceedings Vol. 6268:
Advances in Stellar Interferometry
John D. Monnier; Markus Schöller; William C. Danchi, Editor(s)

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