Presentation + Paper
28 August 2024 Recent technical and scientific highlights from the CHARA Array
Author Affiliations +
Abstract
The Center for High Angular Resolution Astronomy (CHARA) Array is a six-element interferometer with baselines ranging from 34 to 331m. The Array has had many upgrades in recent years including new beam combiners: MYSTIC is a 6T combiner for K-band; SPICA is a 6T combiner for the visible R-band; and SILMARIL is a 3T combiner for high sensitivity in the H- and K-bands. A seventh, mobile telescope is now on site for use with fiber optics for beam transport. Observing time is available to the community through a program funded by NSF. The observing programs are solicited and peer-reviewed by NSF’s NOIRLab. Here we summarize the scientific work and the on-going technical advances of the CHARA Array.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Douglas R. Gies, Narsireddy Anugu, Theo A. ten Brummelaar, Victor Castillo, Christopher D. Farrington, Becky E. Flores, Steven Golden, Jeremy W. Jones, Rainer Köhler, Karolina Kubiak, Cyprien Lanthermann, E. Robert Ligon, Olli Majoinen, Harold A. McAlister, Jayadev Rajagopal, Stephen T. Ridgway, Gail H. Schaefer, Nicholas J. Scott, Nils H. Turner, Norman L. Vargas, Larry Webster, and Craig Woods "Recent technical and scientific highlights from the CHARA Array", Proc. SPIE 13095, Optical and Infrared Interferometry and Imaging IX, 1309502 (28 August 2024); https://doi.org/10.1117/12.3020589
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KEYWORDS
Telescopes

Stars

Binary stars

Beam combiners

Fiber optics

Adaptive optics

K band

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