Douglas R. Gies,1 Narsireddy Anuguhttps://orcid.org/0000-0002-2208-6541,2 Theo A. ten Brummelaar,2 Victor Castillo,2 Christopher D. Farrington,2 Becky E. Flores,2 Steven Golden,2 Jeremy W. Jones,1 Rainer Köhler,2 Karolina Kubiak,2 Cyprien Lanthermann,2 E. Robert Ligon,2 Olli Majoinen,2 Harold A. McAlister,1 Jayadev Rajagopal,3 Stephen T. Ridgway,3 Gail H. Schaefer,2 Nicholas J. Scott,2 Nils H. Turner,2 Norman L. Vargas,2 Larry Webster,2 Craig Woods2
1Georgia State Univ. (United States) 2CHARA Array of Georgia State Univ., Mt. Wilson Observatory (United States) 3NOIRLab (United States)
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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.
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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, 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