Some recent results from the CHARA Array

T. A. ten Brummelaar*, David Huber, K. von Braun, T. Boyajian, N. D. Richardson, G. Schaefer, I. Tallon-Bosc, D. Mourard, H. A. McAlister, N. H. Turner, L. Sturmann, J. Sturmann, J. D. Monnier, M. Ireland

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution


The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.

Original languageEnglish
Title of host publicationResolving the future of astronomy with long-baseline interferometry
Subtitle of host publicationproceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011
EditorsMichelle J. Creech-Eakman, Joyce A. Guzik, Robert E. Stencel
Place of PublicationSan Francisco, CA
PublisherAstronomical Society of the Pacific
Number of pages5
ISBN (Electronic)9781583818596
ISBN (Print)9781583818589
Publication statusPublished - 2014
EventConference on Resolving the Future of Astronomy with Long-Baseline Interferometry - Socorro
Duration: 28 Mar 201131 Mar 2011

Publication series

NameAstronomical Society of the Pacific conference series
PublisherAstronomical Society of the Pacific


ConferenceConference on Resolving the Future of Astronomy with Long-Baseline Interferometry

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