Paper
12 September 2012 Recent technical and scientific highlights from the CHARA Array
Harold A. McAlister, Theo A. ten Brummelaar, Stephen T. Ridgway, Douglas R. Gies, Judit Sturmann, Laszlo Sturmann, Nils H. Turner, Gail H. Schaefer, Tabetha S. Boyajian, Christopher D. Farrington, P. J. Goldfinger, Larry Webster
Author Affiliations +
Abstract
The CHARA Array is a six-telescope optical/IR interferometer managed by the Center for High Angular Resolution Astronomy of Georgia State University and located at Mount Wilson Observatory in the San Gabriel Mountains overlooking Pasadena, California. The CHARA Array has the longest operational baselines in the world and has been in regular use for scientific observations since 2005. In this paper we give an update of instrumentation improvements, primarily focused on the beam combiner activity. The CHARA Array supports seven beam combiners: CHARA CLASSIC, a two-way high-sensitivity K/H/J band system; CLIMB, a three-way K/H/J open-air combiner; FLUOR, a two-way K-band high-precision system; MIRC, a four/six-way H/K-band imaging system; CHAMP, a six-way K-band fringe tracker; VEGA, a four-way visible light high spectral resolution system; and PAVO, a three-way visible light high sensitivity system. We also present an overview of science results obtained over the last few years, including some recent imaging results.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Harold A. McAlister, Theo A. ten Brummelaar, Stephen T. Ridgway, Douglas R. Gies, Judit Sturmann, Laszlo Sturmann, Nils H. Turner, Gail H. Schaefer, Tabetha S. Boyajian, Christopher D. Farrington, P. J. Goldfinger, and Larry Webster "Recent technical and scientific highlights from the CHARA Array", Proc. SPIE 8445, Optical and Infrared Interferometry III, 84450H (12 September 2012); https://doi.org/10.1117/12.926452
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Interferometry

Telescopes

Imaging systems

Planets

Visible radiation

Visibility

RELATED CONTENT

Star and planet formation with the new generation VLTI and...
Proceedings of SPIE (December 13 2020)
An update on the CHARA Array
Proceedings of SPIE (July 21 2010)
CHARA angular diameter measurements with a 330 meter baseline
Proceedings of SPIE (February 21 2003)
Interferometric investigations of highly evolved stars
Proceedings of SPIE (July 05 2000)
An update on the CHARA array
Proceedings of SPIE (July 28 2008)

Back to Top