Rainer Koehler,1 Robert Ligon,1 Matthew D. Anderson,2 Narsireddy Anuguhttps://orcid.org/0000-0002-2208-6541,1 Theo ten Brummelaar,1 Victor Castillo,1 Christopher Farrington,1 Douglas R. Gies,3 Steven Golden,1 Ludovic Grossard,4 Karolina Kubiak,1 François Reynaud,4 Stephen Ridgway,5 Gail Schaefer,1 Nic Scott,1 Laszlo Sturmann,1 Nils Turner,1 Craig Woods1
1The CHARA Array, Georgia State Univ. (United States) 2Georgia Tech Research Institute (United States) 3Georgia State Univ. (United States) 4XLIM (France) 5NSF NOIRLab (United States)
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The Center for High Angular Resolution Astronomy (CHARA) Array currently consists of 6 telescopes at fixed positions, connected by vacuum pipes to the delay lines. The CHARA Michelson Array Pathfinder (CMAP) project includes two major components: 1) a mobile telescope that can be placed at a number of locations, and 2) a fiber optic relay system to transport light to the beam combining facility. The telescope will be equipped with a custom-built instrument bench with adaptive optics and fiber injection. The light will be transported by optical fibers to the existing CHARA delay lines. In this contribution, we present the progress on the various subsystems needed to integrate the new telescope and beam transport method into the existing CHARA environment. We will also describe our efforts to find internal fringes with the new fibers.
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Rainer Koehler, Robert Ligon, Matthew D. Anderson, Narsireddy Anugu, Theo ten Brummelaar, Victor Castillo, Christopher Farrington, Douglas R. Gies, Steven Golden, Ludovic Grossard, Karolina Kubiak, François Reynaud, Stephen Ridgway, Gail Schaefer, Nic Scott, Laszlo Sturmann, Nils Turner, Craig Woods, "Integrating a mobile telescope into the CHARA Array," Proc. SPIE 13095, Optical and Infrared Interferometry and Imaging IX, 1309504 (28 August 2024); https://doi.org/10.1117/12.3020620